The galaxy presents a generally smooth morphology, with a dominant, centrally concentrated bulge. The overall shape appears largely elliptical, approaching circular. There is a suggestion of a faint disk or extended halo component, with a subtle flattening and colour gradient extending outwards from the brighter central region. This outer region appears bluer, contrasting with the redder core. There are no strong indications of spiral arms or significant disturbances to the main structure, with any merging or tidal features being rather minor. The relative colour suggests modest ongoing star formation.
