The galaxy presents as a relatively smooth, elliptical-like structure. Its core appears concentrated and bright, exhibiting a yellowish-white hue that potentially suggests a population of older stars. Surrounding the core is a more diffuse, greenish halo, possibly indicating ongoing or recent star formation. The overall form is largely featureless, without obvious spiral arms or a pronounced disk. The shape is notably round, with no significant elongation detected. There is no readily apparent evidence of active merging or significant gravitational disturbances.
