The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge. The overall color is predominantly yellowish-white, suggesting an older stellar population within. There is a slight asymmetry in the light distribution, with a hint of extended, faint features indicating a possible minor gravitational interaction or previous merger event. The galaxy appears relatively isolated with no other interacting or nearby galaxies visible in the immediate vicinity, which implies a degree of evolutionary maturity. Star formation appears to be at low levels within the visible region, consistent with an older, more evolved system. The galaxy exhibits a round appearance, and the outskirts fade gradually into the background sky.
