The galaxy appears to be a relatively smooth, elliptical system. The central region exhibits a high concentration of light, indicative of a dense stellar population, possibly an older population due to its yellow-orange hue. The isophotes appear largely regular, with a generally elliptical shape. There is little to no evidence of prominent spiral arms or dust lanes. The outer regions display a gradual decrease in surface brightness, with a hint of a faint, diffuse halo. The galaxy shows no obvious signs of recent major merger activity, though subtle tidal features cannot be ruled out at this resolution. There may be minor disturbances in morphology. Overall, it presents as a galaxy dominated by older stars and a quiescent evolutionary state.
