The galaxy presents as an elliptical morphology with a relatively smooth, symmetrical light distribution. The core exhibits a concentrated brightness profile, transitioning smoothly outwards into a more diffuse halo. The color appears consistent across the galaxy's structure, trending towards a redder hue, suggestive of an older stellar population. There are no apparent spiral arms, dust lanes, or other features indicative of recent or ongoing star formation. There is no evidence of any major mergers or tidal disturbances. The galaxy appears relatively isolated in the observed field, with no nearby companion galaxies. The overall appearance is consistent with a massive early-type galaxy at a moderate redshift.
