The galaxy presents as a disk-shaped structure, viewed at an oblique angle, exhibiting a pronounced central bulge. The bulge appears yellowish-white, suggesting a population of older stars. Surrounding the bulge, a fainter disk component extends outward. The disk shows hints of spiral arm structure, though it's not sharply defined. The color of the disk component is bluish-white, suggestive of younger stellar populations and ongoing star formation. There is a moderate degree of smoothness to the overall light distribution, though some irregularities hint at potential disturbances or active star-forming regions within the disk. The galaxy appears to be relatively isolated, without obvious signs of a major merger in progress. The galaxy is elongated, with the major axis more than twice the length of the minor axis. There is a clear fall-off in intensity from the core, as indicated by the central bulge, moving outwards towards the edges of the disk.
