The object appears to be a galaxy, exhibiting a primarily smooth morphology. The overall shape is somewhat elliptical, but deviates slightly from perfectly rounded. There is a faint disk-like structure visible in the central region. Indications suggest a possible minor disturbance or interaction, potentially evidenced by subtle irregularities in the outer regions of the galaxy, though this could also be the result of artifacts. There is no clear evidence of major merging events. The color profile suggests a composition of older stellar populations.
