The galaxy appears to be an elliptical galaxy, possessing a generally smooth and featureless morphology. It exhibits a slightly elongated shape, falling somewhere between round and cigar-shaped. The light distribution suggests a centrally concentrated bulge component that dominates the galaxy's structure. There is no evidence of significant spiral arm structures or a prominent disk. The color gradient indicates an older stellar population that has minimal ongoing star formation. There are no obvious signs of tidal disturbances or interactions with other galaxies, suggesting it is a relatively isolated system, though the presence of close proximity galaxies could suggest a past merging or future event.
