The galaxy presents as a slightly elongated, disk-shaped object with a generally smooth appearance. The light profile indicates a concentration of luminosity towards the center, suggestive of a central bulge. There is a subtle color gradient, with the central region exhibiting a yellowish-orange hue, potentially indicating an older stellar population. The outer regions of the galaxy appear slightly bluer, hinting at the presence of younger, hotter stars, but the overall lack of distinct spiral arm structures or prominent star-forming regions suggests a relatively quiescent state. The galaxy's morphology appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions, though there may be some minor disturbances. The galaxy is generally a cigar shape, with a hint of being in between that and being perfectly round. The galaxy does not appear to be the result of merging.
