This galaxy presents a largely smooth, elliptical morphology. It appears to be relatively round in shape. The central region exhibits a bright, concentrated bulge, indicative of a high stellar density. The outer regions of the galaxy fade gradually, lacking any discernible spiral arm structure or distinct features. The overall color profile leans towards the redder end of the spectrum, suggesting an older stellar population with a lower rate of ongoing star formation. There is no apparent evidence of any major mergers or significant tidal disturbances affecting the galaxy's structure.
