The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. There is little evidence of distinct spiral arms or a prominent disk. The color profile suggests a dominant population of older stars, exhibiting a reddish-orange hue. There may be some signs of minor disturbance or tidal features, but the galaxy is largely undisturbed, showing no indication of a major merger event. The morphology is consistent with that of a relatively massive system. The overall shape is closer to being in between elliptical and round, but has a slight tendency toward elongation.
