The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated luminosity profile. The central region is bright and yellowish, suggestive of an older stellar population. As one moves outward from the core, the intensity gradually decreases, and the color appears slightly bluer, perhaps indicating younger stars in the outer regions. The overall shape is elongated, approximately three times longer than it is wide, with no apparent spiral arm structure or significant dust lanes visible. There is no obvious interaction or major disturbance. There are hints of some disturbances, but these are not a clear indication of merging.
