The galaxy presents as a centrally concentrated, relatively smooth structure. It appears to be an early-type galaxy, likely elliptical or lenticular, with a dominant spheroid component. A defined nucleus is present, exhibiting a high surface brightness. There is no evidence of spiral arms or other distinct disk features. Color gradients are subtle, with the core appearing somewhat yellower than the outer regions, suggesting an older stellar population in the central regions. The overall morphology lacks any significant disturbances or tidal features, and its smooth appearance suggests it is a relatively isolated system that has not undergone any recent major mergers. The galaxy has a consistent and simple shape which may indicate an elliptical shape.
