The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The core region exhibits a yellowish-white hue, suggesting a population of older stars. This color shifts to a bluer tint as it extends outward. This could imply some ongoing star formation in its outer regions. The overall morphology indicates a relatively evolved system with no prominent spiral arms or significant signs of recent major mergers or tidal disturbances. The galaxy appears somewhat rounded with a slight deviation towards a cigar shape.
