The galaxy exhibits a generally smooth morphology, though some finer features are discernible. It appears to be in a transition state between elliptical and spiral, possibly a lenticular galaxy. The galaxy possesses a bright central bulge indicative of an older stellar population. There are some indications of a disk component extending outwards from the bulge; however, any spiral arm structure is poorly defined, and the disk appears rather amorphous.

The color distribution appears somewhat uneven. A redder hue is present within a portion of the disk, potentially indicative of dust lanes or regions of older stars. Bluer colors, which could represent some more recent star formation, appear patchy throughout the disk. There are hints of some tidal interactions or recent minor merger events, visible as subtle distortions in the outer regions of the disk. Overall, it appears to be a galaxy with a mixed stellar population, experiencing a moderate level of star formation, and potentially interacting with a smaller galaxy or experiencing internal dynamical disturbances. The overall shape is mostly round but leans toward an intermediate elliptical shape.
