The galaxy presents as an elliptical morphology with a smooth, diffuse light distribution. The central region exhibits a high concentration of yellow light, suggesting a dominant population of older stars. A smaller, bluer region is observed slightly offset from the main body, potentially indicating a region of ongoing star formation or a smaller interacting companion. The overall structure appears largely undisturbed, showing no signs of major mergers or significant tidal features. The galaxy's color profile suggests that it may be an intermediate-mass system.
