The galaxy presents as a moderately luminous, relatively smooth object. Its morphology appears primarily elliptical, showing a concentrated central bulge that dominates its overall structure. There is a slight elongation, though the object is largely rounded. A faint disk component is possible, but not distinct. The colour profile indicates an older stellar population, dominated by redder wavelengths, with the central bulge being especially pronounced in the longer wavelengths. There may be evidence of a past or ongoing minor interaction, as the outer regions appear slightly disturbed. Overall, it is likely a massive galaxy, with a low specific star formation rate and a high stellar mass.
