The galaxy presents as a moderately luminous object with a generally smooth morphology. A slight elongation is observable, though the overall form leans towards a rounded profile. Color gradients are present, exhibiting a central region with warmer hues, indicative of an older stellar population or a more centrally concentrated star formation activity. The outer regions appear slightly bluer, suggesting the presence of younger stars or ongoing star formation in the galactic disk. Hints of minor disturbances can be seen within its structure. These may be indicative of a past interaction with another galaxy, or tidal effects causing asymmetry. The galaxy appears to have an intermediate mass, and it displays a notable amount of star formation.
