The galaxy presents as a generally smooth, elliptical morphology. It is dominated by a spheroidal component, showing a centrally concentrated bulge that appears round in projection. There are no discernable spiral arms or a prominent disk-like structure. The galaxy exhibits a color gradient, with a yellowish-orange hue concentrated toward the center, suggestive of an older stellar population and minimal ongoing star formation in the core region. The outer regions are less well-defined and appear somewhat bluer, hinting at the presence of some younger, though less prominent, stellar populations in the extended halo. The overall structure is relatively undisturbed, with no obvious signs of a recent major merger or tidal interactions. Minor irregularities or faint extensions are not visible, indicating a dynamically relaxed system.
