This galaxy presents an elongated, cigar-shaped morphology. It appears to exhibit a relatively smooth central bulge with a slightly flattened disk component. The color profile suggests a dominant population of older stars, indicated by the redder hue, although there may be a hint of bluer, potentially younger, stars in the disk. There is a slight indication of internal structure or faint spiral arm segments, but high image noise makes it difficult to determine definitive features within the galaxy. The overall structure appears relatively undisturbed, with no immediately obvious signs of major ongoing mergers. There are also hints of tidal disturbances or faint plumes.
