The galaxy presents a generally smooth and rounded morphology, appearing as an elliptical or lenticular type. A strong central bulge dominates the structure, exhibiting a concentrated and bright core. Fainter and less defined extensions surround this core, fading into the background. The overall color profile indicates a higher concentration of older stellar populations, manifesting as a reddish-yellow hue in the central region, suggestive of lower star formation activity. There are no prominent features indicative of spiral arms or significant dust lanes, and the galaxy appears relatively undisturbed, showing no clear signs of ongoing mergers or tidal interactions with other galaxies.
