The galaxy presents a generally smooth and rounded morphology. The light distribution indicates a central concentration of intensity, suggestive of a prominent galactic bulge. There is only faint evidence of a disk component, but the overall structure appears largely featureless within the limits of the image resolution. The dominant color appears to be reddish-yellow, which could indicate an older stellar population with relatively low levels of ongoing star formation. There is a slight hint of a potential interaction or minor disturbance in the outskirts of the galaxy, but the evidence is not conclusive.
