The galaxy presents as a somewhat symmetrical, elliptical or lenticular structure. Its core region appears bright and concentrated. The color profile suggests a primarily older stellar population, exhibiting a yellow-red hue, especially concentrated in a bright spot that is off-center. The galaxy shows little evidence of spiral arms or significant dust lanes. The outer regions are less defined, gradually fading into the background sky. Based on the light profile, the galaxy has an estimated half-light radius of approximately 6.5 kpc. There may be some minor tidal disturbances.
