The galaxy presents a primarily smooth morphology. The central region exhibits a bright, concentrated luminosity profile suggesting a prominent bulge. The overall shape appears elliptical, with a slight elongation noticeable along one axis, though its classification leans toward round rather than highly elongated. A faint, diffuse halo surrounds the core, gradually fading into the background. There is little evidence of distinct spiral arm structures or significant dust lanes within the galaxy's disk, suggesting it is a relatively evolved system. The colour profile indicates a potentially older stellar population, with a tendency towards redder hues, although a small amount of blue light is detectable within the disk indicating the presence of some recent star formation. There is no indication of major mergers or tidal disturbances, although very minor disturbances cannot be ruled out.
