The galaxy presents a largely smooth and rounded morphology. Its color profile appears generally redder, suggesting a relatively older stellar population. There is no discernible spiral arm structure or evidence of ongoing, significant star formation. The galaxy's compact size and homogenous appearance indicate it's likely an elliptical or S0 type galaxy, and is likely not undergoing any major merging activity. There may be some minor internal disturbances, but the galaxy is generally settled.
