The galaxy appears to be a relatively smooth, elliptical galaxy. Its overall shape is quite round, with no significant elongation or distortion visible. There is a smooth radial profile, indicating a lack of significant spiral arms or prominent disk-like structures. The light distribution appears mostly homogenous. There may be very minor disturbances in the galaxy's morphology, potentially hinting at past or ongoing minor interactions, but any merger activity appears to be negligible. The galaxy exhibits a predominantly redder color, with a lack of strong blue features. This implies that the stellar population is primarily composed of older stars with little ongoing star formation.
