The galaxy exhibits a generally smooth morphology, with a round appearance and a relatively high degree of central concentration. There is little evidence of prominent spiral arms or distinct features suggestive of ongoing major mergers or significant tidal disturbances. The galaxy's light profile is relatively compact, with a characteristic size on the order of several kiloparsecs.

There is a color gradient, with the central region appearing more yellow and the outer regions exhibiting a bluer hue. This suggests that the central region is dominated by an older stellar population, while the outer regions may contain younger, hotter stars and potentially some ongoing star formation, albeit at a relatively low rate. The integrated absolute magnitude suggests that this is a moderately luminous galaxy. It likely contains a significant amount of stellar mass, approximately on the order of 10 to the 11 solar masses.
