The galaxy appears to be elliptical in shape, displaying a smooth, centrally concentrated light profile. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a dominant yellowish-white hue in the central region, suggestive of an older stellar population. Moving outwards, the color transitions to a slightly bluer shade, but this is still relatively subtle. The lack of strong blue colors or distinct features indicates a relatively low star formation rate and a lack of significant recent mergers or tidal disturbances. Overall, the galaxy presents a well-defined, relatively homogenous appearance.
