The galaxy appears to be a relatively smooth, centrally concentrated system with a fairly round morphology. There is a noticeable color gradient, shifting from a more yellow/orange hue towards the galactic center to a bluer tint in the outer regions. The central bulge region seems dominant and exhibits a fairly high surface brightness. Faint, diffuse features appear to extend outwards, suggesting either tidal debris or possible spiral arm structure, although not well-defined. There does not appear to be any strong evidence of ongoing major mergers or significant tidal disturbances. The galaxy's overall appearance is consistent with that of a galaxy undergoing a period of quiescence in terms of major star formation.
