The galaxy presents as a moderately luminous object, appearing somewhat diffuse. Its overall morphology is elliptical, exhibiting a spheroidal shape with a smooth, centrally concentrated light profile. A subtle color gradient is observed, transitioning from a yellowish core to a slightly bluer outer region. There is no evidence of spiral arms or a distinct disk structure. Faint, irregular features or minor disturbances can be seen in the outer regions, possibly indicative of past minor mergers or tidal interactions. Given the color and smooth morphology, the galaxy likely contains an older stellar population, though signs of recent or ongoing star formation cannot be ruled out completely based on the subtle color gradient.
