The galaxy presents as an elliptical morphology, with a smooth, concentrated light profile indicative of an early-type system. The core exhibits a yellowish hue, suggesting an older stellar population dominated by redder giants and dwarfs. The outer regions appear fainter with a slight blue tinge, possibly indicating the presence of younger, hotter stars, although this could be due to image artifacts. There is no distinct spiral arm structure or prominent dust lanes visible. The overall shape is somewhat elongated but generally quite round, with no obvious signs of significant tidal disruption or ongoing major merger events. The system appears relatively isolated and undisturbed.
