The galaxy presents an overall smooth morphology, with a slight elongation but tending toward a rounded shape. The color appears to be primarily yellowish in the central region, possibly indicating an older stellar population. Fainter bluish features are present in the outer regions of the galaxy, perhaps suggesting some ongoing, albeit subdued, star formation. There is a slight asymmetry, or disturbance, in the overall structure. This might be the result of a minor interaction or some internal dynamical process. The galaxy shows no strong evidence of a major ongoing merger or significant tidal disruption in this image. The light from the galaxy is relatively concentrated, appearing less extended in comparison to other galaxies with active star formation regions.
