The galaxy appears as an elongated, cigar-shaped structure, with a noticeable bulge dominating the central region. The bulge exhibits a yellow-orange hue, possibly indicative of an older stellar population. The outer regions of the galaxy display a bluer color, suggesting the presence of younger, hotter stars. There is no apparent spiral arm structure discernible in this image. The galaxy has a smooth appearance, without any major disturbances, plumes, or obvious signs of recent merger activity. The object is relatively faint, with a defined but diffuse edge, and appears to be at considerable distance.
