The galaxy presents a generally smooth and elliptical morphology, with a high degree of central concentration. The core region exhibits a bright, concentrated luminosity profile, suggesting a significant population of older stars. Moving outward from the core, the luminosity gradually decreases into a diffuse halo structure. There's a slight elongation to the galaxy's shape, trending towards a cigar-like form. Faint hints of what may be a disk-like component are visible, though the galaxy is mostly smooth. There is no clear indication of ongoing major merger events or significant tidal disturbances, but it appears as though there may be some minor irregularity in the outer structure on one side. The galaxy exhibits a color gradient from a yellowish core to a slightly bluer halo. This color variation may indicate a diminishing presence of younger, bluer stars in the outer regions.