The galaxy exhibits an overall elliptical morphology, appearing quite smooth and well-defined with a high degree of circular symmetry. It presents a concentrated central bulge that is slightly redder in color compared to the outer regions. The color gradient indicates a potential difference in stellar populations, suggesting that older, redder stars dominate the core.

The galaxy appears relatively isolated with no obvious signs of major interactions or ongoing mergers, although a subtle asymmetry in the outer regions may suggest some minor gravitational disturbance. No distinct spiral arm structures or prominent dust lanes are visible. The overall structure is characterized by a diffuse, extended halo surrounding the brighter central regions. The integrated color suggests the presence of ongoing star formation.
