The galaxy presents as a slightly elliptical, disk-like structure. The central bulge appears to be brighter and more condensed than the surrounding disk. The overall color is skewed toward bluer wavelengths, with the nucleus appearing slightly whiter than the rest of the galaxy. Faint wisps, likely indicative of spiral arms or tidal features, are faintly visible. There seems to be a secondary condensation offset from the central bulge that may represent a potential merger. This is further supported by the galaxy's smooth, yet disturbed appearance. 
