The galaxy presents as a centrally concentrated, relatively smooth object. The core region exhibits a bright, yellowish-orange hue, suggesting a population of older stars. Surrounding the core is a more diffuse halo of greenish light, potentially indicative of ongoing, though likely low-level, star formation or a population of slightly younger stars. The overall shape appears close to elliptical with some irregularity. There does not appear to be a disk-like structure or spiral arms visible in this image, which is consistent with an elliptical morphology. There is little evidence of any major mergers or tidal disturbances.
