The galaxy presents as an elliptical morphology. It has a smooth appearance with a centrally concentrated bulge that emits strongly in the g, r, and z bands. There's no discernable dust lane or spiral arm structure, and the light is fairly uniform, suggesting an older stellar population that is no longer actively forming stars. The galaxy appears relatively isolated, without signs of major tidal disturbances or an obvious nearby interacting companion, though there are faint hints of minor irregularities or extensions in the outer regions. It's a relatively compact galaxy, with an overall smooth luminosity profile.
