The galaxy presents as a relatively smooth, elliptical-like structure. The core region exhibits a high concentration of light, appearing bright and somewhat unresolved at this resolution. Moving outwards, the light gradually diminishes, forming a diffuse halo. The overall color of the galaxy is predominantly yellowish-orange, suggesting a population dominated by older stars. There is a hint of bluer light on the periphery, implying the presence of some younger, hotter stars or perhaps some ongoing, albeit low-level, star formation. There are no obvious spiral arms, dust lanes, or other features indicative of a disk galaxy. The galaxy appears largely undisturbed, showing no clear signs of major mergers or tidal interactions. It has a notably round shape, with no obvious elongation or distortion.
