The galaxy presents a disk-like morphology, viewed at a near edge-on angle. A prominent central bulge is visible, exhibiting a bright, concentrated luminosity. The disk shows evidence of internal structure, with subtle variations in color and brightness suggesting the presence of spiral arms. The galaxy has a slight asymmetry in the luminosity of its disk. Evidence suggests possible minor merger activity. The galaxy's overall color suggests a diverse stellar population with a range of ages. The color in the central region is indicative of older stars. The edge-on orientation and possible minor disturbances make detailed classification challenging.
