The galaxy presents with a compact, centrally concentrated morphology. The light distribution suggests a roughly elliptical shape, though with some noticeable irregularities in the outer regions. A bright central region dominates the overall luminosity profile, possibly indicating the presence of an active galactic nucleus or a region of intense star formation.

The color gradients across the galaxy reveal a possible change in stellar population or dust content. The central region appears bluer, potentially indicative of younger stars or lower dust extinction, while the outer regions are redder. There is a slight indication of a tidal tail, but this could be due to an artifact. It appears the galaxy is undergoing a merger with a smaller object.
