The galaxy presents a generally smooth and rounded morphology, with a concentrated central bulge. The light profile appears relatively uniform, lacking prominent spiral arms or distinct features. The color gradient suggests a predominantly older stellar population, with a reddish hue dominating the inner regions transitioning to a slightly bluer component toward the outer edges. However, it is mostly smooth and yellow. There is no strong evidence of ongoing star formation, such as bright HII regions. Overall, the galaxy appears to be a fairly typical elliptical or S0 type galaxy, exhibiting minimal signs of recent interactions or mergers.