The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated central bulge that gradually fades into a diffuse halo. The color profile suggests a relatively older stellar population, with a subtle shift towards redder hues in the outer regions. No distinct spiral arms or prominent dust lanes are discernible. The overall structure indicates a system with minimal ongoing star formation activity. There is no obvious evidence of major tidal disturbances or interactions with other galaxies.
