The galaxy presents as a largely featureless elliptical or lenticular system, exhibiting a smooth, concentrated light profile that transitions into a more diffuse outer halo. There is little to no evidence of spiral arms or significant dust lanes. The color appears predominantly yellow-orange, suggesting a population of older stars and potentially a lower rate of ongoing star formation. The overall morphology indicates a relatively evolved system, nearing the quiescent end of the galaxy evolutionary sequence. The lack of any tidal features suggests it is likely not undergoing any major interaction, and its shape is closer to spheroidal than disk-like.
