The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, diffuse light distribution with no discernible spiral arm structure. The core region appears bright and concentrated, suggesting a high density of stars. There's a noticeable color gradient, shifting from a yellowish hue in the central bulge to a redder tone in the outer regions, which may indicate an older stellar population in the outer parts. The overall shape is somewhat elongated, more cigar-shaped than perfectly circular. There is no evidence of active merging or major disturbances, although a slight asymmetry might suggest a past minor interaction or disturbance.
