The galaxy presents as a somewhat elliptical structure with a brighter, concentrated central bulge. The color profile suggests an older stellar population dominating the core, indicated by its yellowish hue. Moving outwards from the center, there is a slight shift towards bluer colors within the disk, potentially suggesting more recent star formation in those regions. There is some distortion, but no clear spiral arm structure is apparent. The galaxy does not appear to be undergoing any major merging events or disturbances, although there may be a slight hint of a tidal feature or faint plume extending to the upper left of the galaxy, potentially indicating past or ongoing minor interaction. The overall appearance is relatively smooth, though some subtle texture hints at underlying structure.
