The galaxy presents an elongated, cigar-shaped morphology. A central, bright region exhibits a yellowish-orange hue, possibly indicating an older stellar population or dust attenuation. Fainter, more diffuse regions extend from the central bulge, displaying a slightly greenish tint on one side and reddish on the other. This coloration might be indicative of ongoing star formation within these outer regions. The galaxy appears relatively undisturbed, showing no clear signs of major mergers or tidal interactions, although there is a slight asymmetry. It is likely a massive system with a sizable central bulge, with a low amount of ongoing star formation.
