The galaxy presents as a smooth, elongated structure, generally cigar-shaped. It exhibits a color gradient, transitioning from a bluer hue in its central region to a slightly redder tone towards the outer edges, suggesting potential variations in stellar populations or dust content across the galaxy. The light distribution appears relatively uniform without obvious signs of spiral arms or distinct features and no signs of strong star formation. There is a hint of a disc structure. The galaxy does not appear to be undergoing any major merging activity or significant tidal disruptions, instead it appears to be a system approaching quiescence with a possible low level of star formation.
