The galaxy appears to be a relatively smooth, elliptical-like system. Its color is generally a pale yellowish-white, with a somewhat redder concentration towards the galactic center, suggesting an older stellar population dominating the core. The outer regions exhibit a slightly bluer hue, which may indicate more recent star formation or a younger stellar population present within the galaxy's disk component. The galaxy's overall shape is somewhat elongated, with the ratio of its major to minor axes being approximately 3:1. There is no clear evidence of spiral arms or a prominent bar structure. A slight asymmetry is visible, which could indicate a past or ongoing minor merger event or tidal interaction. The overall morphology suggests an intermediate-mass galaxy with a moderate amount of ongoing star formation.
