The galaxy presents as a somewhat elliptical, smooth structured object. A central bulge is evident, appearing concentrated and yellowish-orange in color, indicating an older stellar population. The outer regions show a subtle, fading greenish-blue hue, possibly suggesting the presence of younger, hotter stars or ongoing star formation within a disk component. There is no strong evidence of spiral arms or significant dust lanes. A slight asymmetry is visible with a possible tidal feature. Overall, the galaxy appears relatively undisturbed.
