The galaxy appears to be a single, gravitationally bound system with a generally smooth morphology. The central region exhibits a bright, concentrated luminosity. Fainter, diffuse light extends outwards, exhibiting a slightly elongated shape, although there is no evidence of a pronounced disk structure. There is some patchy structure apparent in the outer regions of the galaxy, with hints of possible tidal disturbances or ongoing minor mergers. The color profile reveals a central region that is relatively yellow in color, which would suggest an older stellar population, with bluer areas appearing in the outer disk, suggesting more recent star formation.
