The galaxy presents as a relatively smooth, elliptical-like structure. Its core is characterized by a high concentration of light, suggesting a dense stellar population. Moving outward from the center, the light gradually diminishes, forming a diffuse halo. The galaxy's color appears to be generally redder/yellower, potentially indicating an older stellar population with lower ongoing star formation. The overall form of the galaxy appears regular, without obvious signs of spiral arms or major distortions, although there might be some minor disturbances given what looks like a very faint tail. The galaxy exhibits an elongated shape, with the ratio of major to minor axis being approximately 3:1. There is no definitive evidence of a recent or ongoing major merger event.
