The galaxy appears as a moderately bright, relatively smooth object. The central region exhibits a high degree of symmetry, presenting a generally elliptical morphology. There is a slight elongation to the shape, but it leans towards roundness. Some irregularity is observed in the galaxy's structure and it may be undergoing disturbances, possibly from a minor interaction or merger event. There are traces of bluer light in the outer edges, suggesting ongoing star formation, although this activity seems to be primarily concentrated near the galaxy's periphery.
