This galaxy presents as an edge-on spiral, characterized by a prominent central bulge and a flattened disk. The bulge exhibits a smooth, rounded profile, suggesting a relatively old stellar population. The disk appears thin and elongated, with a high degree of symmetry. The color gradient shows a yellowish hue in the central region, likely indicating older stars and a lower rate of star formation. Moving outward along the disk, there is a subtle shift towards bluer colors, implying the presence of younger, hotter stars and ongoing star formation. There is a slight hint of dust lane obscuration along the central plane of the disk. There is no evidence of any major mergers or tidal disturbances, although the galaxy displays a slightly irregular morphology.
