The galaxy presents as a relatively compact object, exhibiting a degree of morphological disturbance. A significant portion of the galaxy's light is concentrated in a central bulge or core region, which appears yellowish-white in color. Emanating outwards from the core are fainter, bluish-white regions which may indicate ongoing star formation.

There is evidence of possible tidal interactions or a minor merger event, indicated by some distortions in the overall shape and the presence of faint plume-like extensions. This suggests a potential interaction with another galaxy or the remnants of a past merger. The galaxy is neither perfectly spherical nor highly elongated, appearing to be in an intermediate stage with some evidence of disruption to its overall shape.
