The galaxy presents a generally smooth, elliptical morphology. It displays a concentrated central bulge with a high degree of sphericity. The color profile indicates a redder core transitioning to bluer outer regions, possibly indicating a gradient in stellar populations, with older, redder stars dominating the center and younger, bluer stars more prevalent in the surrounding areas. There are no immediately apparent spiral arms or a well-defined disk structure. Faint hints of a disturbed morphology are suggested by slight asymmetries in the outer regions. Overall, the object appears relatively isolated, showing no clear signs of ongoing major mergers or strong tidal interactions with companion galaxies. The galaxy is fairly compact and appears well-resolved, presenting a relatively bright, although distant, source.
