The galaxy appears to be a relatively smooth, elliptical-like structure, possibly of an early type. The light is concentrated towards the center with a distinct, bright core, suggesting a high stellar density in the galactic nucleus. The color gradient transitions smoothly from a yellowish-white core to a redder hue in the outer regions. There is little indication of strong spiral arm features or prominent dust lanes. The overall appearance suggests a well-established system with either limited or no recent major merger events, based on the seemingly undisturbed morphology.
