The galaxy presents as a relatively smooth, elliptical structure. It exhibits a distinct central bulge which appears bright and concentrated. The galaxy's color gradient suggests an aging stellar population, with redder hues dominating the core region. There is a general lack of strong spiral arm features or prominent dust lanes. The outer regions of the galaxy are less defined, with a gradual decrease in luminosity towards the edges, forming an apparent halo. The overall morphology indicates a galaxy nearing the end of its star forming lifespan. A faint shell structure is present indicating a possible interaction event in the galaxy's past.&#x20;
