The galaxy presents as a somewhat elongated, cigar-shaped structure. Its central region exhibits a bright, concentrated luminosity, appearing relatively smooth with no obvious spiral arm structures or distinct dust lanes visible. The galaxy's color appears to be mostly red in the DESI color bands, suggesting a stellar population dominated by older stars and potentially a lower rate of ongoing star formation. The outskirts of the galaxy show a gradual decrease in brightness, indicating a transition to lower stellar density at the edges. There is no obvious evidence of tidal tails, strong gravitational lensing, or major merging events in this image, but a potential minor disturbance cannot be entirely ruled out at this resolution.
