The galaxy presents as a relatively smooth object with a predominantly elliptical morphology. It exhibits a high degree of central concentration, appearing almost spheroidal. The color profile indicates an older stellar population, evidenced by the reddish-yellow hue. There is no discernible disk structure or spiral arm features. The galaxy does not show obvious signs of ongoing mergers or significant tidal disturbances, appearing generally undisturbed. A faint halo may be present, but its boundaries are not well-defined.
