The galaxy presents a generally smooth, elliptical morphology, elongated along a principal axis. The light profile suggests a centrally concentrated bulge, characterized by a yellowish-white hue indicative of an older stellar population. Moving outward from the core, the luminosity gradually decreases, transitioning to a more diffuse and reddish outer halo. This halo appears less structured than the central region, with a subtle fading into the background sky. There is no clear evidence of spiral arms or significant dust lanes. The overall appearance is consistent with a relatively quiescent galaxy, likely experiencing a low rate of star formation. Subtle irregularities within the outer halo might suggest minor tidal interactions, but the dominant impression is one of a relaxed, evolved system.
