The galaxy appears to be a relatively smooth, elliptical system. Its central region exhibits a concentrated, yellowish-orange hue, suggestive of an older stellar population. Moving outward from the core, the color gradient shifts towards a slightly bluer, albeit still subdued, tint. The overall morphology suggests a spheroid-dominated structure with a subtle disk-like component viewed at an oblique angle. There are no readily apparent signs of strong tidal interactions or major mergers, although subtle disturbances cannot be ruled out. The galaxy's color profile and smooth appearance indicate a system that may be undergoing a period of quiescence in terms of star formation.
