The galaxy presents as a generally elliptical object with a smooth, relatively homogenous light distribution. The core region exhibits a higher surface brightness, with the overall color appearing to be shifted towards the red end of the spectrum. This color suggests a population dominated by older stars and minimal ongoing star formation. There are disturbances that indicate possible recent merging activity or tidal interactions. The presence of a secondary component hints that this might be either an active galactic nuclei or a tidal effect from two combined galaxies. It appears relatively compact, with no discernible spiral arms or prominent dust lanes visible in this image.
