The galaxy presents a predominantly smooth morphology, exhibiting a lack of prominent spiral arms or distinct features. Its shape appears to be somewhere between round and elliptical. The galaxy displays a central bulge with a concentrated luminosity gradient, suggesting a relatively old stellar population dominating the core. 

The overall color index indicates a redder spectral energy distribution, consistent with a population of evolved stars. There is a faint, diffuse halo surrounding the central region that may contain some minor tidal disturbances. The galaxy does not appear to be undergoing a major merger. The galaxy is moderately large. 
