The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. There is a notable absence of distinct spiral arm structures or prominent dust lanes, suggesting a population dominated by older stars. The color profile exhibits a redder hue, concentrated towards the galactic center, potentially indicating an aging stellar population and reduced recent star formation activity. The overall shape appears slightly elongated, but lacks any obvious signs of major mergers or significant tidal disturbances. The galaxy shows a possible faint outer halo.

