The galaxy presents as an elongated, disk-shaped structure viewed at a steep inclination. It exhibits a centrally concentrated bulge with a yellowish hue, potentially indicative of an older stellar population. The outer regions of the disk appear bluer, suggesting ongoing or recent star formation. The galaxy appears relatively smooth in overall texture, with little evidence of spiral arm structure or significant dust lanes visible in this image. There may be a slight asymmetry in the galaxy's shape, though it's difficult to determine from this image whether it's intrinsic to the galaxy or a result of projection effects. There appear to be no major merger events underway and no apparent tidal tails or distorted morphologies.