The galaxy appears as a single, centrally concentrated object with a generally smooth morphology. The light distribution suggests an elliptical shape. The central region exhibits a bright, yellowish hue, potentially indicative of an older stellar population. Fainter, bluer regions extend outwards, although the overall color profile suggests a relatively quiescent galaxy with modest star formation. There are no signs of strong tidal interactions or major disturbances in its structure. Evidence suggests that the galaxy is not undergoing a major merger.
