The galaxy presents an elongated, cigar-shaped morphology, suggesting it is likely an elliptical galaxy, possibly of type E4-E7. The light distribution appears smooth and centrally concentrated, with a gradual decrease in surface brightness towards the edges, with a possible bulge. There appears to be little or no evidence of spiral arms, prominent dust lanes, or ongoing star formation regions visible in this image. The galaxy exhibits a pale yellowish to white color in the central regions, possibly indicating an older stellar population. The overall observed color suggests the presence of a stellar population composed predominantly of older, redder stars, with a corresponding low rate of current star formation. Given the observed redshift, this galaxy is at an intermediate distance and appears to be a mid-sized galaxy in terms of physical extent.
