The galaxy appears to be elliptical in shape, displaying a smooth, centrally concentrated light distribution. The color profile suggests a relatively evolved stellar population, with a dominant yellowish-red hue in the core and a gradual fading toward the outer regions. There is little evidence of distinct spiral arm structure or significant dust lanes. No signs of major mergers or strong tidal disturbances are readily apparent, although the possibility of minor interactions cannot be ruled out based on this single image. The galaxy presents a regular, symmetrical morphology.
