The galaxy appears as a relatively smooth elliptical or lenticular structure. Its light is generally concentrated towards the center, diminishing towards the edges, indicative of an older stellar population. The galaxy presents a somewhat round morphology, with a slight suggestion of elongation but without prominent spiral arm structures. There may be subtle disturbances suggesting potential past interactions, but without any major disruption of the overall structure. The galaxy color is reddish, indicating a significant population of older stars, and a low ongoing star formation rate.
