The galaxy presents as a relatively smooth, elliptical object. Its morphology suggests it is likely an early-type galaxy, potentially an elliptical or lenticular system. The light distribution is centrally concentrated, with a gradual decrease in surface brightness extending outwards from the core. The axial ratio indicates a moderate ellipticity, appearing somewhat cigar-shaped rather than perfectly circular. There is a very slight indication of a possible faint disk structure. Overall, the galaxy's appearance indicates a system dominated by older stellar populations, with minimal evidence of ongoing or recent major star formation activity and no signs of any prominent merger event. The color gradients suggest the central regions may be slightly redder than the outer regions.
