The galaxy presents a generally elliptical morphology, appearing relatively smooth and concentrated. It exhibits a bright, yellowish central bulge, suggesting a significant population of older stars. Fainter, bluish extended features surround the core, possibly indicating regions of ongoing star formation, although they are not clearly resolved into distinct spiral arms. The overall shape is somewhat rounded, without any obvious signs of major tidal disturbances or ongoing mergers, although subtle irregularities in the outer regions cannot be ruled out. The galaxy's color gradient, from yellow in the center to bluer at the edges, suggests a radial distribution of stellar populations, with older, redder stars dominating the core and younger, bluer stars residing in the outer disk.
