The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The color profile leans heavily toward the red end of the spectrum, suggestive of an older stellar population. The lack of distinct spiral arms or prominent dust lanes supports its classification as an early-type galaxy. There appears to be little evidence of recent or ongoing major mergers or tidal disturbances. A slight asymmetry in the outer isophotes could hint at minor interactions, or could simply be an artifact of observation. The galaxy exhibits a moderately compact structure with a relatively high surface brightness in its core, fading into the background sky.
