The galaxy appears as a roughly circular, centrally concentrated object. The light profile suggests a relatively smooth distribution. A bright, compact core is observed, surrounded by a more diffuse halo or bulge component.

The core exhibits a redder color compared to the surrounding halo which appears bluer, implying a possible difference in stellar populations. It appears that the bulge dominates over the disk. There is a possibility of a minor interaction given the slight irregularity. The roundness of the galaxy suggests it is not highly inclined.
