The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge, which graduates into a fainter, more diffuse halo. The color profile suggests an older stellar population, appearing reddish-orange. There's a slight elongation, deviating marginally from a perfect circular shape. No prominent dust lanes or spiral arm structures are discernible within the galaxy's morphology. The overall appearance indicates a lack of ongoing major star formation, with a dominant population of evolved stars. There's no visual evidence of any significant merger events or tidal disturbances affecting the galaxy's structure.
