The galaxy presents as an elongated, cigar-shaped structure. Its light profile appears relatively smooth, lacking distinct spiral arm features or a prominent central bulge. The core of the galaxy exhibits a reddish-orange hue, suggesting a population of older stars and possibly significant dust obscuration. The outer regions appear bluer, potentially indicating the presence of younger, hotter stars. There's a hint of asymmetry or a minor disturbance on one side, which might be indicative of a past or ongoing interaction with another galaxy or internal processes affecting the galactic structure. Overall, the galaxy appears to be a moderately massive system, likely an elliptical or lenticular type, located at a considerable distance.
