The galaxy presents a somewhat amorphous morphology. It appears predominantly smooth in structure, displaying a central concentration of light with a slight elongation. The overall form is roughly rounded but with discernible disturbances to its circular symmetry, suggesting possible interactions or internal activity. There is a suggestion of internal features or merging systems. The color profile indicates a moderate amount of ongoing or recent star formation, contributing to its overall brightness. The galaxy is of significant mass, and its light reveals a substantial stellar population.
