The galaxy presents as a flattened, cigar-shaped structure. It exhibits a smooth, diffused morphology with no distinct spiral arms or prominent features readily visible. The central region shows a higher concentration of light, appearing more luminous and potentially indicative of a galactic bulge. The color gradient suggests a redder core, possibly composed of older stellar populations, transitioning to slightly bluer hues towards the outer edges, hinting at more recent star formation in those regions. There is no noticeable dust lane obstruction. The galaxy does not display any strong signs of ongoing interaction or merging events.
