The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually fades into the outer regions. No distinct spiral arms or bar structures are readily apparent in this image. The color profile suggests a population of older stars, as indicated by the reddish-yellow hue. There are only very minor disturbances or tidal features, suggesting the galaxy has not undergone a major merger in recent history. The overall shape is generally round, without significant elongation. The galaxy appears relatively isolated, showing no obvious signs of interaction with neighboring galaxies or clusters. 
