The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated central bulge that dominates its overall structure. The light is yellowish-white, indicative of an older stellar population. There is no apparent spiral arm structure or significant dust lanes. The galaxy has a somewhat elongated shape, and the outer regions show a decrease in luminosity, with an extended halo. The color of the halo seems to be shifting towards the redder wavelengths. There is no distinct sign of tidal features or ongoing major mergers. 