The galaxy presents as a predominantly smooth, elliptical morphology. The light distribution is centrally concentrated, exhibiting a gradual decrease in intensity from the core outwards. There's a hint of some faint, diffuse structures, suggesting possible interactions or tidal features, but these are not prominent. The color profile indicates a somewhat passive stellar population, showing a significant presence of older, redder stars. The galaxy appears relatively isolated, with no immediate evidence of ongoing major mergers. There's no visually apparent dust lane or spiral arm structure. Overall, it appears to be a relatively quiescent elliptical galaxy, with a smooth light profile.
