The galaxy presents as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge that graduates outwards to a more diffuse halo. The central bulge is distinctly brighter and appears to be composed of older stellar populations, indicated by its yellowish-white hue. There is a subtle color gradient moving outward from the core, showing a slight shift towards bluer tones in the outer regions, suggesting younger, more luminous stars. The overall shape is moderately elongated, but not significantly so, displaying an "in-between" form between round and cigar-shaped. No prominent spiral arms, dust lanes, or other distinct features are observable, suggesting a lack of active star formation. There are no indications of ongoing or recent major mergers or significant disturbances. The structure is consistent with an early-type galaxy that is likely to be quiescent.
