The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The light profile appears to decline steadily from the center outwards, suggesting a lack of prominent spiral arms or significant star-forming regions readily visible in this image. The overall color appears to be on the redder side, indicative of an older stellar population dominating the galaxy's luminosity. There are no obvious signs of ongoing major mergers or tidal disturbances. The galaxy exhibits a high degree of central concentration and ellipticity, but the outskirts fade gradually into the background, indicating a diffuse halo or envelope of stars.
