The galaxy presents as a fairly smooth, elliptical-like structure with a concentrated central bulge. The galaxy exhibits a generally round morphology, lacking any obvious spiral arm features or a pronounced disk. There is a slight indication of a minor disturbance in its overall shape, but it does not appear to be undergoing a major merger. Color gradients across the galaxy are subtle, with a tendency toward redder hues towards the outer regions, suggesting a potentially older stellar population in these areas. The galaxy's light is dominated by a smoothly distributed component, with no clear signs of prominent star-forming regions.
