The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a concentrated central bulge that appears yellowish-white in color, suggesting a population of older, redder stars. The galaxy's overall shape is elongated, displaying an intermediate ellipticity that is neither perfectly round nor highly elongated. A faint disk is visible around the bulge. No prominent spiral arm structures or significant dust lanes are discernible. The galaxy lacks obvious signs of ongoing major mergers or tidal disturbances. A subtle color gradient is observable, with the central regions exhibiting a more yellow hue, transitioning to slightly bluer tones towards the outer edges.
