The observed galaxy presents as a centrally concentrated object, exhibiting a roughly elliptical morphology. A bright, compact core dominates the galaxy's luminosity profile. The core transitions into a slightly more diffuse outer region. The object appears relatively smooth in texture with minimal discernible substructure, suggesting it is likely to be an early-type galaxy or a spiral with a dominant bulge. There are indications of minor disturbances present, likely a very slight distortion of the galaxy's overall shape, but not definitive signs of any major ongoing merger events.
