This galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge, characterized by a yellowish-white hue, indicative of an older stellar population. The galaxy's overall shape is somewhat flattened, appearing between round and cigar-shaped, suggesting a degree of rotational support. There's little evidence of significant disk features or spiral arms. The galaxy's light profile fades gradually from the center outwards, with the outer regions displaying a bluer tint, possibly due to a younger stellar population or some ongoing, albeit subdued, star formation activity. No signs of major mergers or significant tidal disturbances are apparent, suggesting a relatively isolated and undisturbed evolutionary history.
