The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The overall color is yellowish-white, possibly indicating a population of older stars. There are very faint hints of a disk component, but the image largely suggests a spheroid-dominated morphology. There appears to be no significant spiral arm structure or major dust lanes visible. There is no evidence of any recent or ongoing major merging events, or any signs of major disturbance. The galaxy appears well-defined, suggesting a generally relaxed and evolved system.
