The galaxy exhibits a generally smooth morphology, with a centrally concentrated bright region. There is a relatively smooth transition in brightness from the core outwards, with no distinct spiral arms or bar structures apparent. The object appears ellipsoidal, though nearing a circular shape, with some elongation. The light distribution suggests the galaxy is dominated by an older stellar population, as evidenced by the yellowish-red hue of the central bulge. There is little evidence of ongoing major star formation. There may be some very minor asymmetries or disturbances in the outer regions, but the galaxy does not obviously appear to be strongly interacting or undergoing a major merger.
