The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, appearing nearly circular in projection. The color gradients suggest a stellar population with a slightly higher concentration of older, redder stars toward the center and a subtle bluer population in the outer regions. The overall color is slightly red, typical of galaxies with low star formation rates. There is no evidence of significant spiral arm structure or a prominent disk. The galaxy does not show any obvious signs of recent major mergers, although subtle disturbances or minor interactions cannot be ruled out.
