The galaxy exhibits a complex morphology, suggestive of an ongoing or recent merger event. There are two distinct luminous regions. The primary region displays a smoother, more elliptical profile, while the secondary region appears more irregular and possibly disk-like. The color variation within the galaxy is subtle, but there is evidence of bluer regions and redder regions. The blue regions are concentrated in the disk-like area, indicating ongoing star formation. The redder regions seem to be in the elliptical primary region, possibly indicative of an older stellar population. There may be tidal tails or faint extended features emanating from the galaxy indicating gravitational interaction. The galaxy does not appear to have a single well-defined nucleus, reinforcing the merger hypothesis.
