The galaxy presents an elliptical morphology, appearing largely smooth and featureless. There is a concentrated central bulge of high luminosity with a radial decrease in surface brightness. The galaxy exhibits a slightly elongated shape, transitioning from round to cigar-shaped. No apparent spiral arm structures, dust lanes, or signs of ongoing major merger events are detectable within the resolution limits of the image. Minor disturbances may be present, but a relaxed and evolved system is the dominant visual impression. The galaxy appears redshifted suggesting a considerable distance. The galaxy exhibits a range of colors, with the central core exhibiting redder hues, suggesting an older stellar population. Star formation may occur at a low rate. The estimated mass range is significant and typical of an older galaxy.
