The galaxy presents as a diffuse, moderately bright object with an apparent elliptical morphology. A significant portion of the light appears smoothly distributed, but there are indications of possible disturbances. It is likely experiencing an episode of star formation. There is a redder component visible at the edge, which could indicate a region with older stars or dust obscuration. The object does not appear particularly isolated, suggesting the possibility of interactions with nearby galaxies. Overall the galaxy appears generally normal with the faint possibility of a minor merger.
