The galaxy presents as a centrally concentrated object, with a smooth, largely featureless morphology. The light distribution suggests a spheroidal shape, transitioning from a bright, compact core to a fainter, diffuse halo. Color gradients are subtle but present, with the central region appearing more blue-white, possibly indicating a population of younger, hotter stars. The outer regions exhibit a redder hue, suggestive of an older stellar population. There is no obvious evidence of spiral arms, bars, or tidal features in the visible light, nor is there any indication of strong dust lanes. The object displays a slightly elongated, but overall rounded shape. No signs of any major merging events, or disturbances are observed.
