The galaxy presents as a relatively smooth, centrally concentrated system. The morphology appears to be elliptical, exhibiting a bulge-dominated structure with minimal evidence of spiral arms or disk features. The core is bright, suggesting a high concentration of stars and potentially a supermassive black hole at the center.

The color gradient is primarily yellow to red, indicating a population of older stars. The redder hue implies a paucity of ongoing star formation and a dominance of evolved stellar populations. The galaxy shows no signs of significant tidal disturbances or interactions with neighboring galaxies. It appears to be a relaxed, evolved system.
