The observed galaxy presents as a late-type spiral system viewed nearly edge-on. A prominent dust lane is visible, bisecting the galaxy's bulge and disk. This dust lane absorbs and obscures light from the regions behind it, contributing to the dark band seen along its length. The central bulge exhibits a yellowish hue, suggesting an older stellar population. The disk shows a gradient in color, transitioning from a brighter, more yellow-toned region near the center to bluer, less luminous areas further from the core. This may indicate ongoing star formation in the outer regions of the disk, where younger, hotter stars are prevalent. The galaxy's light profile appears smooth and somewhat centrally concentrated, with a moderately declining surface brightness outward from the nucleus. Overall, the galaxy displays characteristics consistent with a disk-dominated system, potentially exhibiting a low-luminosity active galactic nucleus, based on its magnitude.
