The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with luminosity decreasing gradually toward the outer edges. The core is dominated by yellow and orange hues, potentially indicating an older stellar population. There is a notable absence of defined spiral arms or significant dust lanes. Faint extensions of light are visible, with a subtle asymmetry in its shape, possibly due to a minor gravitational interaction or tidal disturbance in the past. Overall, the galaxy's morphology suggests a classification as an early-type galaxy with no significant star formation currently.