The galaxy presents as a centrally concentrated object with an elliptical morphology. It exhibits a smooth light distribution, lacking prominent spiral arms or significant substructure. The overall color appears yellow-orange, suggesting a population of older stars, potentially with minimal ongoing star formation. The galaxy's roundness indicates a probable E0-E3 classification on the Hubble sequence. There is no visual evidence of tidal tails or other features indicative of recent or ongoing major mergers, although some minor disturbances cannot be entirely ruled out based on this image alone. The galaxy's core appears unresolved at this resolution.
