The galaxy presents as a flattened, disk-like structure with a prominent central bulge. The luminosity profile appears to be smooth, with a gradual decrease in brightness from the core outwards. The color gradient suggests a population of older stars dominating the central region, as evidenced by the yellowish hue. Fainter, bluer regions are observed within the disk, potentially indicative of younger stellar populations and ongoing star formation. The overall shape is elongated, showing a cigar-like appearance. There is no apparent evidence of any major disturbances or tidal features indicative of recent major merger activity, however there may be a minor disturbance. A faint, small companion is also observed. 
