The galaxy presents as a somewhat elongated, centrally concentrated object. It exhibits a relatively smooth morphology, with the majority of its light emanating from a defined, bright core. The central region displays a yellowish-white hue, suggesting a population of older stars.

Surrounding the core, a more diffuse, bluish halo is observed. The blue color indicates the presence of a younger stellar population and possibly ongoing star formation. The distribution of this bluer component appears somewhat uneven, lacking a well-defined spiral structure. The overall shape is closer to elliptical, but with hints of a disturbed or irregular form. Evidence for a disk is weak. There may be minor disturbances present in its structure but no major merging is indicated.
