The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity moving outwards, characteristic of early-type galaxies. There is no clear evidence of spiral arms or a disk structure. The color profile suggests a dominant population of older stars, contributing to the overall reddish-yellow hue. No significant dust lanes or active star-forming regions are visibly apparent. The overall structure appears undisturbed, with no obvious signs of recent major merger events or tidal features. The galaxy appears to be a single, relatively isolated system.
