This galaxy presents as a relatively smooth, elongated structure, suggesting an elliptical morphology or a spiral galaxy viewed edge-on. There is a notable concentration of luminosity towards the center, indicative of a prominent galactic nucleus. The light distribution gradually decreases moving outwards from the center.

There appears to be little to no evidence of distinct spiral arm structures or significant dust lanes. The galaxy exhibits a color profile that leans toward the redder end of the spectrum, which typically corresponds to a stellar population dominated by older, redder stars. This could imply a relatively low rate of current star formation.

There are no obvious signs of tidal disturbances or ongoing mergers. The overall appearance suggests a relatively evolved and quiescent galaxy, lacking the features associated with active star formation or recent interactions.
