The galaxy exhibits a largely smooth morphology, with a high degree of central concentration. It appears elliptical in shape, being close to round, with only a slight deviation towards an elongated form. There is no visual evidence of spiral arms or a prominent disk structure. The galaxy presents a color gradient, transitioning from a yellowish-white core to a bluer, diffuse halo. There's little indication of recent major mergers or tidal disturbances, although subtle asymmetry in the outer regions cannot be ruled out. Overall, the galaxy appears to be a relatively quiescent system, likely dominated by an older stellar population with a relatively low rate of star formation.
