The galaxy presents as a relatively smooth, concentrated object. It appears mostly elliptical. There's a moderate amount of light concentration in the galaxy's center, with a smooth luminosity gradient decreasing towards the outer edges. The galaxy appears to have a mass on the lower end. Its star formation rate seems to be correspondingly low. It appears to have undergone little disturbance from mergers, which fits with its smoother appearance. The color profile shows a slightly redder hue near the center compared to the edges, potentially indicating a higher concentration of older stars in the core.
