The galaxy presents as a relatively smooth, elliptical morphology. It displays a concentrated, bright central bulge that transitions gradually into a more diffuse halo. The color profile suggests an older stellar population, with a yellowish-red hue dominant throughout the galaxy, indicating a lack of significant recent star formation activity. The galaxy exhibits a high degree of rotational symmetry. No distinct spiral arm structures or prominent dust lanes are discernible, further supporting the classification as an elliptical galaxy. There is no obvious indication of any tidal distortions or interactions with neighboring galaxies.
