The galaxy appears as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated, bright yellow core, suggesting a high density of older stellar populations. Moving outwards from the core, the color transitions to a redder hue, which may indicate slightly younger populations. The overall roundness of the galaxy is fairly regular, with a minimal cigar shape. The galaxy shows no obvious signs of major disturbances or ongoing mergers, appearing largely isolated and quiescent. There may be some minor asymmetries or faint features that need a higher resolution image to resolve.
