The galaxy presents as a flattened spheroid, displaying characteristics intermediate between a pure elliptical and a spiral galaxy when viewed from this angle. The central bulge appears bright and relatively smooth in texture, suggesting a high concentration of older stars. Fainter, bluer regions are observed extending along the major axis, potentially indicating areas of more recent star formation within a disk-like structure. The disk itself appears relatively faint and not well-defined. The overall color is intermediate, trending toward the redder end of the spectrum, which further indicates an aging stellar population. The observed ellipticity is significant, hinting at possible past or ongoing interactions influencing the galaxy's morphology. No distinct spiral arms are visible. There appears to be some degree of disturbance in the outer regions, possibly indicating past interactions.