The galaxy appears to be a relatively smooth, elliptical-type galaxy at a moderate redshift. The galaxy exhibits a concentrated, bright central bulge, which gradually fades into a less luminous, extended halo. The isophotes appear somewhat elongated, suggesting a shape that is intermediate between a perfect sphere and a flattened disk. There is no apparent spiral structure or strong dust lane visible in the image. The overall color of the galaxy is yellowish, indicating a stellar population that is dominated by older, redder stars. There is no evidence of ongoing major mergers or significant tidal disturbances affecting its overall structure, although a small possibility of a minor disturbance cannot be ruled out. The galaxy appears fairly isolated, without any close companions or signs of strong interactions with other nearby galaxies in the immediate vicinity.
