This galaxy presents as a smooth, elongated structure, lacking defined spiral arms or a prominent central bulge. The light distribution appears relatively uniform across its surface, with a slight concentration towards the center. Its color profile suggests a population of older stars and a reduced rate of active star formation. There is an absence of any major disturbances to its form, suggesting it is not currently undergoing a major merger or interaction. The overall morphology is consistent with an elliptical galaxy, but its slightly elongated shape could also indicate a lenticular type.
