The galaxy appears as a moderately luminous, relatively compact object. Its overall morphology is smooth, suggesting an elliptical or lenticular classification. The light distribution is centrally concentrated. There is a marginal asymmetry in the shape. Color gradients are apparent, with the central region exhibiting a slightly bluer hue compared to the outer regions, potentially indicating the presence of some younger stellar populations or an active galactic nucleus. There are no obvious signs of spiral arms or prominent dust lanes. The object does not appear to be undergoing a major merger event, though there is a slight irregularity in the disk structure that could suggest minor tidal interaction.
