The galaxy presents a largely smooth, elliptical morphology. It has a concentrated central bulge, characterized by a reddish-yellow hue, suggesting a population of older stars. The galaxy exhibits a gradual decrease in luminosity outwards from the core. There is minimal evidence of spiral arm structures or significant dust lanes. Overall, this appears to be a relatively undisturbed system. The light profile indicates a high degree of central concentration, with a lack of significant tidal features or distortions that would suggest recent major merger activity. There may be some very faint, diffuse outer structures but the resolution is too low to determine the exact nature.
