The galaxy appears to be a relatively smooth, elliptical system. Its central region presents a reddish hue, potentially indicative of an older stellar population. Moving outwards from the core, the color shifts toward a slightly bluer/greenish tint, suggesting the presence of some younger, hotter stars, though not in significant quantities.

The galaxy exhibits a moderately concentrated profile, fading gradually from the center outwards. There are no clear signs of spiral arms, bars, or significant dust lanes. Its overall shape is somewhat elongated, but it does not appear excessively flattened or cigar-shaped. There is no readily apparent evidence of ongoing major mergers or significant tidal disturbances. The overall morphology suggests a galaxy that is evolving relatively passively.
