The galaxy presents a generally smooth and rounded morphology. Its color profile suggests a dominant population of older stars, exhibiting a yellowish-red hue that is most concentrated towards the center. There is some evidence of a faint, greenish tint in the central region, which may indicate some ongoing, though limited, star formation. No distinct spiral arm structure or prominent dust lanes are visible. There is a slight irregularity to the shape, but it is generally well-formed and unperturbed. The overall appearance is indicative of a fairly massive, evolved system, likely an elliptical or lenticular galaxy.
