The galaxy presents as a relatively smooth, elliptical structure. Its color profile indicates a strong central concentration of yellow light, suggesting a significant population of older stars. The outer regions exhibit a bluer hue, indicative of some ongoing, though limited, star formation. The overall shape appears largely undisturbed, showing no strong signs of tidal interactions or major merger events, although there may be a subtle disturbance in the distribution of light on the outer edge. The galaxy is relatively compact, with a concentrated light profile.
