The galaxy presents as a lenticular or possibly an elliptical galaxy, with a smooth, diffuse light profile and no discernible spiral arm structure. The central bulge appears prominent and elongated. The overall shape is cigar-like, indicating an axis ratio significantly deviating from unity. Color gradients are subtle, but the central region appears slightly yellower, suggesting an older stellar population compared to the outer regions, which exhibit a bluer tinge. There is no evidence of significant tidal disturbances or ongoing major mergers, though minor asymmetry cannot be ruled out. The galaxy shows a consistent, relatively uniform surface brightness, which suggests a relatively stable morphology.
