This galaxy exhibits an elliptical morphology, appearing generally smooth and concentrated. The core region is bright and concentrated, possibly indicating a higher density of older stars or perhaps the presence of an active galactic nucleus, though the resolution does not allow for definite determination. Moving outwards from the core, the light gradually diminishes, showing an extended halo. The overall color appears to be somewhat redder, suggesting a stellar population dominated by older, redder stars. There's a slight elongation in its shape, appearing somewhat flattened rather than perfectly spherical, and it doesn't appear to have any signs of major ongoing mergers or tidal disturbances, though faint disturbances are not out of the question. A slight amount of bluer color is visible in the outer regions, potentially indicating some recent star formation, albeit at a relatively low level. The overall texture is smooth, with no distinct dust lanes or spiral arm features visible.
