The galaxy presents as a centrally concentrated elliptical, appearing largely smooth with minimal observable substructure or features. Its shape tends towards an oblate spheroid, slightly elongated, with an axial ratio suggesting it is not perfectly circular. The core region exhibits a bright, concentrated luminosity gradient, indicating a high stellar density. Moving outwards, the galaxy gradually decreases in surface brightness. There is a subtle color gradient observed, where the central bulge seems to have a yellow-orange hue, while the outer regions exhibit a slightly bluer tone, this may indicate older stellar populations in the center and younger stellar populations toward the edges. This color distribution could also be affected by dust. There is no evidence of spiral arms, bar structures, or significant tidal disturbances or ongoing mergers within the limits of the image resolution.
