The galaxy presents a moderately smooth profile, though there are subtle features suggesting internal structure. Its overall shape appears somewhat elliptical, but not perfectly round. The galaxy exhibits a central concentration of light, with a gradual decrease in brightness towards its outer regions. There are hints of diffuse, fainter structures extending from the main body, possibly indicative of tidal interactions or ongoing mergers. Patches of bluer light, interspersed with more yellow-red regions, indicate varying stellar populations and potentially active star formation within the galaxy. The overall impression is that of a galaxy undergoing some degree of interaction or disturbance, evidenced by the subtle irregularities in its shape and luminosity distribution.
