The galaxy presents as a somewhat elliptical structure, though close to being in between elliptical and round. The central bulge appears prominent, exhibiting a concentrated luminosity gradient. There is a discernible disk component, exhibiting a subtle color contrast relative to the bulge. The color of the disk appears bluer, potentially indicating the presence of a younger stellar population. The galaxy's appearance is largely undisturbed, with no major signs of ongoing mergers or significant tidal features. The galaxy exhibits an absolute magnitude suggesting that it is a luminous galaxy. The data estimates the mass of the galaxy as moderately high. Based on the star formation rate, the galaxy is actively forming new stars, though not at an exceptionally high rate.
