The galaxy presents an elliptical morphology with a smooth, diffuse light distribution. A prominent central bulge dominates the structure, exhibiting a concentrated, yellowish-white hue, likely indicative of an older stellar population. Fainter, bluer light extends outwards from the core, suggesting the presence of some younger stars or regions of ongoing star formation. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or major mergers. Its overall shape appears to be tending to roundness, and there may be an extremely subtle, almost cigar-like appearance due to the angle we view the galaxy. 
