The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, transitioning into a more diffuse halo region. The core of the galaxy appears yellowish-orange, suggesting a population of older stars. Faint hints of bluer light are visible in the outer regions of the galaxy, potentially indicative of a small amount of ongoing star formation. No prominent spiral arms or a well-defined disk structure are apparent. The overall morphology suggests a system that has largely exhausted its gas supply, resulting in a low star formation rate. There is no evidence of major mergers or tidal disturbances in the observed image. The galaxy's shape is generally round, with minimal elongation or asymmetry.