The galaxy presents a largely smooth, elliptical morphology. It appears highly rounded in shape, showing minimal deviation from circular symmetry. A prominent, bright central bulge dominates the overall structure, characterized by a yellowish-orange hue. This suggests a stellar population dominated by older, redder stars, and a relative lack of ongoing star formation in the central region. The intensity of the bulge decreases gradually with radial distance. There is no discernible spiral arm structure or prominent dust lanes visible in the image. The galaxy exhibits a relatively compact profile, with no evidence of major tidal disturbances or ongoing mergers with other galaxies. The overall appearance suggests an evolved system, likely a massive elliptical galaxy with a high degree of morphological regularity.
