The galaxy presents an elliptical morphology with a smooth, centrally concentrated light distribution. Its core region exhibits a yellow-white hue, indicating a population of older stars. Moving outward from the core, the color gradually shifts towards a redder tone, suggesting a possible decrease in stellar age or an increase in dust obscuration. There is little evidence of prominent spiral arms or active star formation regions in the visible spectrum. The overall structure appears largely undisturbed, without significant signs of ongoing mergers or tidal interactions.
