The observed galaxy presents as a lenticular or possibly a spiral galaxy viewed at a significant inclination. It exhibits a bright, concentrated central bulge, surrounded by a flattened disk. Within this disk, there are regions of varying luminosity, indicating some non-uniform distribution of stellar populations or dust. 

Distinct color gradients are present. The central bulge appears more yellow-white, suggesting an older stellar population. The disk exhibits a bluer tint, indicating the presence of younger, hotter stars. There is a hint of possible spiral arm structure or dust lanes, which are subtle but visible. The overall morphology suggests that the galaxy may have undergone some interaction or disturbance in the past, possibly a minor merger, although the overall structure appears relatively well-defined and not significantly disrupted. 
