This galaxy presents a generally smooth, elliptical morphology. The color profile shows a concentration of yellow and gold hues towards the galactic center, suggesting an older stellar population dominates the core region. This central region appears relatively dense. The outer regions exhibit a more diffuse appearance with fainter intensity. There appears to be minimal, if any, structured features such as spiral arms or a prominent disk component. The galaxy's overall shape approximates a rounded structure, with only subtle deviations from perfect circularity. There is no strong evidence of ongoing major mergers or significant tidal disturbances, although some minor irregularities could be present in the faint outer regions. The red color suggests moderate redshift and potentially a substantial distance from the observer. Overall, the galaxy appears to be a passively evolving system with characteristics consistent with an elliptical galaxy composed of older stars.
