The galaxy presents a largely smooth, elliptical morphology. It appears to be quite rounded in shape, with a bright, concentrated central region, likely representing a dense galactic nucleus. The galaxy exhibits a yellow-orange hue, suggestive of an older stellar population and a lack of significant ongoing star formation. There is some subtle variation in color across the galaxy, with hints of redder regions possibly indicating areas of dust or older, cooler stars. No distinct spiral arms or bar structures are apparent. There may be evidence of a very minor disturbance, but the overall structure appears relaxed and well-defined. Based on the observed redshift, this galaxy is at a significant cosmological distance. The galaxy is relatively massive.
