The galaxy presents a primarily smooth morphology, suggestive of an elliptical galaxy or a spiral galaxy viewed at a high inclination. It exhibits a central bulge region that appears elongated with a moderate ellipticity. The color gradient transitions from a redder hue in the central bulge to a bluer color in the outer regions. The galaxy lacks any obvious spiral arm structures or strong dust lanes. There is some potential for a faint disk component that may be contributing to the overall shape and bluer hue of the outer regions. No obvious signs of ongoing major mergers or significant tidal disturbances are observed.
