The galaxy presents a largely smooth, centrally concentrated morphology. It appears somewhat elliptical in shape, though close to circular, lacking any obvious strong disk features or spiral arms. The light distribution shows a gradual decrease in intensity from the bright nucleus outwards, suggesting a significant bulge component. There is some evidence of a fainter, diffuse halo extending beyond the core, but no prominent tidal features or indications of a recent major merger are visible. Subtle color variations are present across the galaxy's body with an apparent bluer hue to the outer regions compared to the central yellowish core. This color gradient might indicate ongoing star formation towards the edges. Slight asymmetry is also observable, potentially suggestive of a minor disturbance or interaction. Overall, the galaxy appears to be a relatively massive system with evidence of both an older stellar population in the core and some more recent star formation in its outer parts.
