The galaxy presents as a somewhat elongated, cigar-shaped structure. The central region exhibits a bright, concentrated luminosity suggesting a high density of stars or an active galactic nucleus, though the resolution does not permit definitive determination. The light profile fades gradually from the core outwards. The outer regions appear smoother with less clear boundaries, but there seems to be evidence of disk like features at the left, and some areas of more recent star formation on the right. The galaxy color is more red/yellow than blue, indicating an older stellar population. There is no obvious presence of spiral arms or bar structures, but the presence of an ongoing or recent merger cannot be ruled out. The galaxy appears relatively isolated within the field, without any immediately adjacent interacting companions.
