The galaxy appears to be a relatively small, early-type system, likely an elliptical galaxy. The light distribution is concentrated toward the center, with a smooth, diffuse profile, exhibiting a lack of distinct features. The morphology is generally elongated, but nearly round, with the light gradually fading outward from the bright central region. There is a subtle color gradient present, with the central region appearing more yellowish-white and the outer regions tinged with a faint blue hue, suggesting a possible population of younger stars in the outer parts of the galaxy. The lack of spiral arms or significant dust lanes indicates that the galaxy is not actively forming many stars, and has likely undergone several mergers. No signs of interactions with neighboring galaxies are visible.
