The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity outwards. The light profile appears largely uniform with no distinct spiral arm structures visible. The color indices suggest a population of older stars, likely with a low rate of ongoing star formation. There is no obvious sign of a recent major merger or strong tidal disturbances; however, the possibility of minor disturbances cannot be ruled out. The shape is generally rounded, tending towards elliptical rather than a highly elongated form.
