The galaxy presents as a moderately luminous object, exhibiting a generally smooth morphology, although subtle features can be discerned. The light distribution indicates a possible disk structure with a prominent bulge. It has a central concentration of light suggesting an older stellar population, likely located within the bulge. There may be a minor interaction or merging event occurring, suggested by asymmetry and tidal disturbances present. The galaxy shows a slight elongation, but mostly appears round. The color gradients suggest the presence of regions with different stellar populations or dust content. There may be some star formation, although it does not seem to be a vigorous starburst galaxy. Overall, the galaxy appears to be a relatively evolved system undergoing possible interactions.
