This galaxy exhibits a primarily disk-like morphology, although a significant bulge component is evident. The central bulge appears bright and spheroidal, exhibiting a yellowish hue, suggesting an older stellar population.

The disk appears relatively smooth, with limited indication of well-defined spiral arms or distinct star-forming regions. The outer regions of the disk gradually fade into the background, indicative of lower stellar density. The overall color of the disk leans toward a slightly redder hue. The smooth features indicates an elliptical morphology.

Based on morphology and color profile, the galaxy likely has a substantial stellar mass, with a low rate of star formation. There is no strong indication of significant tidal distortions or ongoing major merger events. There is no visible dust.
