The galaxy presents a relatively smooth, elongated morphology, appearing cigar-shaped. A distinct central bulge exhibiting a yellowish hue is prominent, suggesting an older stellar population dominates this region. Fainter, bluish colors are observed extending outward from the central bulge, possibly indicating the presence of younger, hotter stars within a disk-like structure. The overall structure is relatively undisturbed, with no apparent signs of major mergers or significant tidal disturbances. There may be some minor disturbances though. The galaxy exhibits a general smooth appearance, implying minimal recent star formation activity.
