The galaxy appears to be a relatively smooth, elliptical type, exhibiting a flattened, cigar-shaped morphology. Its light distribution is centrally concentrated, with a gradual decrease in surface brightness towards the outer regions. While a disk cannot be excluded, it does not appear to be very prominent. There is no discernible bulge, spiral arm structure or intense star-forming regions visible in the image. Overall the galaxy is a quiescent system, with little to no signs of mergers.
