The galaxy presents a generally smooth, elliptical morphology, exhibiting a concentrated central bulge. There is a slight elongation, deviating marginally from a perfectly circular form. The galaxy's color appears reddish-yellow, indicating an older stellar population with relatively low rates of ongoing star formation. The light is centrally concentrated, which could suggest a significant population of older stars within the bulge. There is no discernible evidence of spiral arms, a prominent disk structure, or any major disturbances indicative of a recent or ongoing merger. The overall form is consistent with an elliptical galaxy that is not currently undergoing any significant interactions.
