The galaxy presents a generally elliptical morphology. It exhibits a smooth appearance with a concentrated central bulge. Faint, diffuse extensions are observed, giving it a somewhat lenticular appearance. The color profile suggests a dominant population of older stars, indicated by its yellowish central region. The outer regions show hints of blue, implying some level of ongoing, though limited, star formation. There is no obvious indication of a major merger, but the slight asymmetry and faint extensions could imply past minor interaction. The galaxy appears to be relatively isolated.
