The galaxy presents as a yellowish-white elliptical structure. It exhibits a generally smooth morphology, with a high degree of central concentration of light. There is a slight elongation noticeable, hinting at a deviation from perfect circularity, though overall, the shape approaches a rounded form. No obvious spiral arms, dust lanes, or significant features indicative of ongoing star formation are immediately apparent. The galaxy appears relatively undisturbed, lacking signs of major mergers or significant tidal disruptions, although minor disturbances or interactions cannot be entirely ruled out at this resolution. The galaxy's color suggests an older stellar population, and potentially minimal current star formation activity.
