The galaxy presents as a relatively smooth, elliptical-like structure. The core appears to be a concentrated, bright region with a yellowish-orange hue, suggestive of an older stellar population. Moving outward from the center, the light gradually fades into a more diffuse halo. There are no apparent spiral arms or prominent dust lanes. A faint blue tint is visible on the outskirts of the galaxy, indicating a possible presence of some younger, hotter stars, though to a small extent. The overall morphology implies a system that is not undergoing major mergers, and is likely a fairly relaxed system with limited active star formation currently taking place. The estimated size is on the larger side, indicating a substantial galaxy in terms of spatial extent.
