The galaxy appears as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that transitions smoothly into an extended, diffuse halo. The light profile suggests a lack of prominent spiral arms or a well-defined disk, instead presenting a more spheroid-like morphology. The central region displays a yellowish-orange hue, possibly indicating a population of older stars and/or dust obscuration. Moving outward, the color appears to become slightly bluer, suggesting the presence of some younger stellar populations in the outer regions, though the overall color is not strongly indicative of active star formation. There is no obvious evidence of a major ongoing merger or significant tidal disturbances. The galaxy appears generally undisturbed.
