The galaxy presents a roughly elliptical morphology. A brighter, seemingly spherical central bulge is evident, surrounded by a fainter, more diffuse halo. There is evidence of a disk structure, exhibiting a slight degree of rotational symmetry, seen edge-on. Within the disk, some regions appear to be less smooth, possibly indicating the presence of dust lanes or spiral arm segments. However, the overall structure of the disk is not clearly defined, and may be disrupted. The dominant color is a bluish hue, potentially indicating the presence of younger, hotter stars. Signs of a potential minor disturbance or interaction are present, but the galaxy does not appear to be undergoing a major merger event.
