The galaxy presents as a somewhat elliptical, smooth, and centrally concentrated system. The core appears quite bright and featureless, gradually fading into a more diffuse halo. There is little evidence of spiral arms or distinct morphological features. The galaxy exhibits a slight elongation. The color profile suggests an older stellar population, with a redder central region transitioning to slightly bluer hues in the outer regions. The galaxy does not appear to be undergoing any major mergers or significant tidal interactions. There may be very minor disturbances, but it mostly exhibits a relaxed morphology.
