The galaxy presents as a relatively smooth, elliptical-like structure. It has a concentrated central bulge that appears to be spheroidal and dominates the overall luminosity profile. The light profile falls off gradually from the center outwards. The galaxy exhibits a yellow-white hue, which could indicate an older stellar population. There is minimal evidence of spiral arms or active star formation regions. No significant disturbances or ongoing mergers are immediately apparent, but there is some low level evidence of a possible minor disturbance. It appears fairly round, with a diameter of around 3.4 kpc. Overall, this appears to be a fairly massive galaxy with relatively little star formation.
