The galaxy appears to be of an elliptical morphology. It is characterized by a high degree of central concentration with a smooth light profile, suggestive of an older stellar population. The central region exhibits a yellowish hue, potentially indicative of older, redder stars. Extending outward from the core, there is a faint, greenish halo of diffuse light. The outer regions gradually fade into the background sky with no clear boundary. The galaxy's shape is roughly circular. There may be some faint tidal disturbances present in the form of asymmetry, potentially hinting at past or ongoing interactions with other galaxies. However, this is not a clear indication of a merger.