The galaxy exhibits a flattened, elliptical morphology, appearing intermediate between a perfectly circular and a highly elongated shape. A central bulge is evident, displaying a concentrated luminosity. The overall color profile suggests an older stellar population, with a dominant yellowish-orange hue. Faint, diffuse arms or features are discernible beyond the bright central region, indicative of a possible disk structure, though not sharply defined. There is minor asymmetry or irregularity, hinting at possible past interactions or ongoing internal processes. The galaxy does not appear to show any signs of a major ongoing merger or tidal disruption in this image.
