The galaxy presents as an elliptical or lenticular system due to its smooth, relatively featureless morphology. It exhibits a centrally concentrated luminosity profile. The primary body is a rounded shape, with a slight deviation towards an elongated structure but not significantly cigar-shaped. There appears to be a subtle distortion or minor disturbance, possibly indicative of past or ongoing interactions. There are no distinct spiral arms visible, the galaxy is dominated by a homogenous light distribution. Color gradients suggest a population of older stars, primarily emitting in the redder wavelengths. The overall impression is a system in a relatively advanced stage of evolution, with indications of a high stellar mass and low specific star formation rate.
