The galaxy appears to be a relatively compact object, exhibiting a generally smooth morphology. The light distribution suggests a centrally concentrated structure, with a radial falloff in surface brightness. It displays a nearly circular shape, with minimal deviation from rotational symmetry.

There is a subtle indication of potential tidal disturbance or interaction, possibly indicated by a faint plume-like extension extending from the main body of the galaxy. This feature is subtle, but potentially suggests minor gravitational interactions with other nearby galaxies. The galaxy exhibits a color gradient, with bluer hues concentrated more towards the central region, while the outer regions appear redder.
