The galaxy presents a somewhat irregular morphology. It displays both a diffuse, smooth component and a more defined, disk-like structure. The central region exhibits a bright, concentrated luminosity, possibly indicative of an active galactic nucleus or a region of intense star formation.

A faint disk-like structure appears to extend outward, oriented in a near edge-on configuration. The color gradient along this feature suggests a distribution of stellar populations, with bluer hues potentially indicating younger stars and ongoing star formation, contrasting with a redder, more evolved population. There is a suggestion of minor tidal disturbances or asymmetries in the faint outer regions, possibly hinting at past interactions or mergers.

The overall color profile suggests that it is a moderately massive galaxy with a moderate amount of star formation.
