The galaxy presents as a relatively smooth, elongated structure. Its morphology suggests it is likely an elliptical galaxy, with a cigar-like shape dominating its visual appearance. There is a smooth central concentration of light, indicating a nucleus. The color gradient transitions from a bluish hue in the outer regions to a more yellowish-white core. This may imply a mix of younger stellar populations in the outer regions with older, redder stars dominating the central bulge. There is a lack of distinct spiral arm structures or prominent dust lanes visible in the image. Minor disturbances are possible, but the overall structure remains relatively undisturbed.
