The galaxy presents as a centrally concentrated, elongated structure. Its overall color profile suggests an older stellar population, with a yellow-orange hue dominating the central bulge. The galaxy exhibits a relatively smooth appearance, lacking prominent spiral arms or significant dust lanes. The shape is closer to cigar-shaped than perfectly round. There is no indication of ongoing major merger events or significant tidal disturbances from other galaxies. Subtle color gradients can be observed, with the central region appearing slightly more yellow compared to the outer regions of the galaxy. The galaxy appears to be at a considerable distance, based on its angular size and redshift.
