This galaxy presents as a roughly elliptical structure, appearing mostly smooth. Its color profile is primarily concentrated in the redder bands, suggesting an older stellar population and potentially lower ongoing star formation. There is subtle evidence of some disturbance or features within the disk, but this is not conclusive. The galaxy does not appear to be undergoing a major merger, although there may be minor tidal interactions or disturbances affecting its overall structure. The shape of the galaxy is moderately elongated, falling somewhere between round and cigar-shaped.
