The galaxy presents as a centrally concentrated object, with a smooth, somewhat elliptical morphology. The light is dominated by a bright, central bulge region, exhibiting a yellow to white hue. There is some suggestion of a fainter, more diffuse disk component extending outwards. The overall color suggests an older stellar population, with ongoing, but relatively low, star formation. There may be some minor irregularity or disturbance in the structure, though it is not a clear merger event. The galaxy appears relatively isolated with no obvious signs of major tidal interactions. The estimated size is a few kiloparsecs across.
