The galaxy appears to be an elliptical galaxy, characterized by its smooth, featureless morphology and elliptical shape. It exhibits a concentrated central bulge that transitions smoothly outward. There is a strong radial gradient in surface brightness, with the core being significantly brighter than the outer regions. The galaxy appears to be relatively isolated, with no obvious signs of major mergers or tidal disturbances. There are hints of a disk, but this is largely dominated by the elliptical morphology. The overall color is fairly uniform, suggesting an older stellar population with little ongoing star formation.
