The galaxy appears as a relatively compact object with an apparent size on the order of a few arcseconds. It exhibits a centrally concentrated light profile, with a bright, possibly unresolved core. Surrounding the core is a fainter, more diffuse halo or envelope.

The color of the galaxy is predominantly blue-green, particularly within the core and inner regions. This suggests a relatively young stellar population and ongoing star formation. The outer regions appear slightly redder, which may indicate the presence of older stars or dust obscuration.

There is some evidence of irregularity in the galaxy's outer shape, with a subtle hint of asymmetry in the isophotes. This could be indicative of a minor interaction or disturbance, though the galaxy's overall structure seems generally intact. No strong tidal features or other signs of major merging activity are apparent.
