The galaxy appears as a centrally concentrated elliptical system. It exhibits a generally smooth morphology with a high degree of radial symmetry, lacking any readily apparent spiral arms or bar structures. The color profile suggests a dominant older stellar population, evidenced by the redder hue concentrated in the core and a gradual shift toward slightly bluer tones moving outward from the center. The isophotes are generally elliptical, with a moderate ellipticity indicating a shape somewhere between round and elongated. There is no visible evidence of ongoing major mergers or significant tidal disturbances, although some subtle asymmetry in the outer halo region cannot be completely ruled out based on this image alone. The relatively smooth light distribution implies a well-mixed stellar population, suggesting a long period of dynamical relaxation since any major formative event. The galaxy likely possesses a substantial stellar mass. Based on the color profile and smooth morphology, the galaxy likely has a relatively low star formation rate.
