The galaxy presents as an elliptical or lenticular morphology, with a significantly brighter central bulge region indicative of a concentrated stellar population. A faint, diffuse disk is potentially visible, however, the system is likely bulge-dominated. The object appears relatively smooth in texture, showing only subtle variations in brightness across the structure. The color profile suggests a evolved stellar population, with a yellow to reddish hue. There's an absence of prominent spiral arms or significant dust lanes. No signs of active galactic nuclei or strong star formation are visually apparent in this image. The object exhibits moderate ellipticity, implying a deviation from perfect circularity. There are no visible tidal tails or other obvious signs of a major merger event, though subtle disturbances might be present within the disk.
