The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a somewhat elliptical morphology, appearing to be moderately round. There's a slight elongation, but it's not strongly cigar-shaped. The galaxy's color profile suggests an older stellar population, with a redder central region transitioning to a slightly bluer halo. There is no evident strong spiral arm structure or significant dust lane presence. There are no obvious signs of ongoing major mergers or significant tidal disturbances in this image, although some minor disturbance is plausible. Overall, it appears to be a galaxy on the more massive end, with low to moderate star formation.
