The galaxy presents as a single, concentrated light source with a generally smooth profile. It appears elliptical in shape, though not perfectly round, exhibiting a slight elongation. The central region displays a high surface brightness, suggesting a dense concentration of stars or an active galactic nucleus. Moving outwards from the core, the light gradually fades, indicating a decreasing stellar density. There is no obvious spiral structure or distinct features readily apparent in this observation, such as prominent dust lanes or star-forming regions. The color appears yellowish-white, likely indicating a stellar population dominated by older stars. The overall appearance suggests a mature galaxy, possibly an elliptical or lenticular type. There is no clear evidence of ongoing mergers or significant tidal disturbances.
