The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. Its color profile suggests an older stellar population, with a yellow-red hue dominant in the central regions. There appears to be a subtle bluer component hinting at ongoing, but low level, star formation. The overall shape indicates a high degree of symmetry, lacking any obvious signs of significant tidal disturbances or major mergers. It exhibits a notable lack of prominent spiral arms or dust lanes. The galaxy seems to be relatively isolated.
