The galaxy presents a flattened, elliptical morphology. The central bulge appears smooth and concentrated, with a yellowish hue, suggesting an older stellar population. Extending outward from the bulge is a fainter disk, exhibiting a bluer color, indicative of younger stars and potentially some star formation. The disk appears relatively featureless with only a few subtle signs of spiral structure, and is tilted at an angle, giving it a cigar-shaped appearance. The galaxy appears relatively isolated, with no obvious signs of major mergers or tidal disturbances.
