The galaxy presents as a moderately bright, elliptical-like structure with a dominant bulge. The luminosity appears to be fairly uniform, with the central bulge showing a slightly more concentrated brightness. There is little to no evidence of spiral arms or disk-like features. Color gradients suggest that the central region may be comprised of an older stellar population compared to the outer regions. The galaxy displays a smooth morphology, with no obvious signs of tidal disturbances or ongoing mergers. The overall shape can be characterized as being somewhere between rounded and cigar-shaped.
