The galaxy appears to be a relatively smooth elliptical galaxy with a somewhat centrally concentrated brightness profile. Its color is predominantly yellow-orange, indicating a population of older stars and a lower rate of ongoing star formation. There is little evidence of spiral arms or a distinct disk structure, further supporting its classification as an elliptical galaxy. The galaxy exhibits a moderate degree of roundness, being neither perfectly spherical nor highly elongated. There are no obvious signs of major mergers or significant tidal disturbances in the immediate vicinity, although subtle asymmetries may indicate minor past interactions. Overall, the galaxy presents a picture of a mature, relatively quiescent system.
