The galaxy presents an overall smooth morphology with a possible slight elongation, appearing somewhat cigar-shaped. The core region exhibits a yellowish hue, possibly indicating a population of older stars. The galaxy appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. There might be some minor disturbances, as can be detected by subtle uneven distribution of light. It may have relatively low specific star formation rates and is likely a massive galaxy.
