The galaxy appears as a relatively smooth, elliptical-like structure with a concentration of light towards the center, suggesting a prominent bulge. The color profile shows a tendency towards redder hues in the core, potentially indicating an older stellar population. There's a subtle gradient toward bluer colors in the outer regions, which might be evidence of ongoing, albeit limited, star formation activity. The galaxy appears isolated, showing no obvious signs of major interactions or mergers with other galaxies, though there is a very faint disturbance noted. The shape deviates slightly from a perfect sphere, appearing somewhat elongated. Overall, it presents as a mature, relatively quiescent galaxy with characteristics of an elliptical or lenticular type.
