The galaxy appears as a relatively smooth, elliptical object. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The color profile suggests an older stellar population, with a dominant yellowish-red hue, particularly within the core. There is little evidence of spiral arm structure or significant dust lanes. The galaxy's shape is moderately elongated, presenting an intermediate ellipticity. No signs of ongoing major mergers or tidal disturbances are discernible, though some minor irregularities in the outer profile could indicate past interaction.
