The galaxy presents a generally smooth and rounded morphology. It exhibits a central bulge, appearing somewhat redder in color, which could indicate an older stellar population. A faint, diffuse disk-like structure surrounds the bulge, showing a bluer hue, suggestive of ongoing or recent star formation. Some subtle features or disturbances are visible, although they do not appear to be indicative of a major merger event. Overall, the galaxy appears to be relatively isolated and undisturbed.
