This galaxy exhibits a morphology that is neither purely elliptical nor a well-defined spiral. There appears to be a central bulge region characterized by a relatively high surface brightness, appearing nearly spheroidal and smooth in texture. Surrounding this bulge is a fainter, more diffuse disk component. The disk component appears to exhibit some degree of structure. There is some slight indication of arm-like structures or irregular features within the disk, however these are not strongly defined. Overall, the galaxy appears moderately inclined with respect to our line of sight, but not perfectly edge-on. There is no strong evidence of a major merger event, although there could be some minor tidal distortions or interactions visible in the outer regions of the disk. The overall color of the galaxy is somewhat redder, particularly within the central bulge, but with blue features possibly along the spiral arms. The outer disk regions appear bluer than the central bulge, perhaps indicating younger stellar populations there.
