The galaxy presents as a slightly elongated, singular object with a smooth, elliptical morphology. The central region appears brighter and more concentrated, with a color gradient transitioning from a yellowish hue in the core to a slightly bluer tint in the outer regions. There is no discernable dust lane, spiral arm structure, or other distinct features indicating recent or ongoing major mergers. The overall form suggests a relatively evolved system dominated by an older stellar population with moderate mass and a suppressed star formation rate. Marginal disturbance may be present, although it's uncertain without more comprehensive imaging.
