The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated morphology. The central bulge is prominent and appears yellowish-white, suggesting a population of older stars. The outer regions of the galaxy fade gradually into the background, indicating a lack of distinct spiral arms or significant dust lanes. The galaxy exhibits a slight elongation, appearing cigar-shaped rather than perfectly spherical. No apparent signs of recent major mergers or tidal disturbances are observed, though there could be some minor asymmetry. Overall, the galaxy presents a regular and relatively undisturbed structure.
