The galaxy appears to be a relatively smooth, elliptical galaxy, with an absence of distinct spiral arms or a pronounced disk structure. The light is concentrated towards the center, indicating a bulge that is mostly spheroidal. The galaxy appears to be fairly round. There is little evidence of significant tidal disturbances or ongoing merging activity, as its shape is fairly regular and undisturbed. Color gradients suggest a population of older stars, particularly toward the central bulge. Overall the galaxy presents as a typical early-type system, with a generally smooth morphology and no significant star formation.
