The galaxy presents as a relatively compact object with a smooth, concentrated morphology. The light profile suggests an elliptical or lenticular classification. The galaxy exhibits a color gradient, with a reddish-orange core transitioning to a yellower halo. This color difference could be indicative of an older stellar population concentrated in the core, with younger stars spread throughout the galaxy. There is a faint bluish area to the left of the core, that could indicate some younger, hotter stars that have formed more recently. There is little evidence of spiral arms, dust lanes, or other distinct features typical of spiral galaxies. There is no indication of any ongoing merger activity, although there might be minor disturbances or interactions. Overall, the galaxy appears to be a fairly mature system, potentially quiescent in terms of star formation.
