The galaxy presents a dominant, centrally concentrated bulge component, appearing smooth and elliptical in shape. There's a slight elongation, suggesting it may not be perfectly spherical. Faint hints of a disk-like structure are present, but the bulge clearly dominates the overall morphology. The galaxy exhibits a color gradient, with the central regions appearing more yellow or orange, indicative of an older stellar population. Towards the outer regions, there's a slight shift towards bluer hues, suggesting more recent star formation. It is possibly interacting with an adjacent galaxy. There's a visual suggestion of tidal disturbances or faint plumes extending away from the main body, though it is difficult to say for sure without a wider field of view and deeper imaging. Overall, the galaxy is a complex system that is still forming stars and likely has a significant mass. 
