The galaxy presents an elongated, cigar-shaped morphology. Its light distribution appears to be largely smooth, with a concentrated central bulge that emits a yellowish hue, indicative of an older stellar population. The outer regions of the galaxy exhibit a bluer tint, suggesting the presence of younger, hotter stars, although the blue light is not prominently distributed. The overall structure suggests a disk galaxy, though lacking distinct spiral arms. There is no visual evidence of a major ongoing merger or significant tidal disturbance. Faint disk structures are seen, which could indicate active star formation, or may simply be a more diffuse region of the galaxy.
