The observed galaxy exhibits a moderately inclined disk-like morphology. There is a suggestion of a disturbance or tidal feature. The central bulge appears somewhat prominent and elongated along the major axis, displaying a yellowish-orange hue indicative of an older stellar population. The disk itself shows a bluer color, especially in the outer regions, indicating recent or ongoing star formation. Faint dust lanes are suspected within the disk, though the image resolution limits definitive identification. There appears to be another galaxy, possible satellite, slightly above this galaxy, possibly indicating an interaction. The overall smoothness of the galaxy suggests that the majority of its stellar mass is contained within the disk and bulge, with little evidence of a prominent spiral structure or irregular morphology.
