The galaxy presents as a relatively smooth, centrally concentrated object. It has an elliptical morphology, appearing more rounded than elongated. The core of the galaxy exhibits a bright, yellowish hue, suggesting a population of older stars. Moving outward from the center, the color gradually shifts towards a bluer tone. There is a lack of any distinct spiral arm structure or prominent dust lanes. The overall light distribution suggests a fairly uniform stellar population within the galaxy's body, with a possible slight flattening towards the edges. There does not appear to be evidence of any major ongoing mergers or significant tidal disturbances affecting the galaxy's structure. The system seems relatively quiescent and evolved.
