The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a bright, concentrated central bulge with a gradual decrease in luminosity towards its outer edges. The galaxy appears nearly round with a hint of ellipticity. Faint extensions or tidal features are not readily apparent, suggesting it is not currently undergoing a major merger event, although there may be minor gravitational disturbances. The colour profile indicates an older stellar population with yellow and red hues dominating the central region, while the outer edges show some evidence of bluer stars, indicating ongoing star formation at a low rate. Overall, this appears to be a massive galaxy with a high mass concentration.
