The galaxy presents as a centrally concentrated object, exhibiting a predominantly smooth morphology. The light distribution is noticeably concentrated towards the center, which shows a pronounced, bright core region. The outer regions of the galaxy appear more diffuse and less structured. There's a hint of bluish tint surrounding the inner core suggesting presence of younger stellar population. Faint, indistinct structures may exist in the outer halo, but the image resolution limits clear discernment. The overall shape of the galaxy approximates a rounded form, with a minor deviation towards slight elongation. There is no immediately apparent evidence of strong tidal interactions or ongoing merger events. The central region's luminosity suggests a well-developed bulge component, which is somewhat luminous. Overall, the image depicts a galaxy with characteristics leaning toward an elliptical or lenticular classification.
