The galaxy presents as a smooth, elliptical structure with a pronounced central bulge. The light distribution suggests a concentration of older stellar populations, indicated by the yellowish-red hue, especially in the central region. There is minimal evidence of spiral arms or significant dust lanes within the observable structure. The galaxy is moderately luminous, with a smooth gradient extending from the bright core to the fainter outer regions. There may be a hint of a very faint disk, as its shape is slightly elongated rather than perfectly circular. The overall impression is of an evolved galaxy lacking active star formation. Slight asymmetries in the outer light distribution could potentially indicate past or ongoing minor interactions.
