The galaxy presents a primarily smooth, elliptical morphology, with a high degree of central concentration. The color profile indicates an older stellar population, with a yellow to red hue dominating the central bulge region. There appears to be a faint disk extending beyond the bright central bulge, though the disk structure lacks well-defined spiral arms. The overall shape is more in between round and cigar shaped than either extreme. There is no immediately clear evidence of a major ongoing merger event. There appears to be a region of bluer, more recent star formation in an off-center location away from the main body of the galaxy, though star formation activity is generally low. This galaxy appears to be a relatively massive system.
