The galaxy presents a generally elliptical morphology, appearing more elongated than perfectly spherical. A bright, concentrated central bulge is evident, exhibiting a yellowish hue, possibly indicative of an older stellar population. Fainter, disk-like extensions emanate from the central region, showing a subtle color gradient towards bluer tones, hinting at ongoing star formation. The overall structure appears relatively undisturbed, lacking prominent tidal features or signs of major mergers. The galaxy is likely a massive system, displaying a degree of smoothness and a limited presence of distinct features such as spiral arms or prominent dust lanes.
