The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. A pronounced bulge dominates the central region, exhibiting a yellowish-white hue, suggesting an older stellar population. Moving outwards from the core, the galaxy transitions to a bluer color, indicating the presence of younger, hotter stars. The outer regions show a less defined structure, with a gradual fading into the background sky, indicating a decrease in stellar density. There are hints of faint, irregular extensions or tidal features in the outer regions, particularly on the right side, suggestive of past or ongoing gravitational interactions. The overall appearance is that of a relatively evolved galaxy with a significant spheroidal component. 
