The galaxy presents a morphology characterized by a combination of smooth and featured components. The overall structure appears somewhat elliptical, though not perfectly round, with a hint of elongation along one axis. A central bulge is discernible, exhibiting a bright, concentrated luminosity. Surrounding the bulge, a fainter, more diffuse disk component is visible.

Evidence suggests ongoing or recent interactions or merging events. Irregularities in the galaxy's shape and light distribution are noted, potentially indicating tidal disturbances or the presence of smaller, merging companion galaxies. The color profile reveals a mix of stellar populations, with bluer regions indicative of recent star formation, and redder regions suggestive of older stellar populations.
