The galaxy appears as a centrally concentrated, roughly elliptical structure. It exhibits a smooth, diffuse morphology with no obvious spiral arm features or dust lanes visible in this observation. The overall color profile is yellowish, indicating a stellar population dominated by older, less massive stars. The galaxy appears relatively isolated with no other merging galaxies in close proximity. Some minor disturbances can be noted, but they do not indicate a major merger in progress. The round shape and lack of defined structure suggests that the object is an elliptical galaxy, a classification that is consistent with its smooth appearance and color.
