The galaxy exhibits a generally elliptical morphology, although it appears somewhat disturbed or asymmetric. A central, brighter region suggests a concentration of stars toward the galactic nucleus. The overall color is slightly blue-tinged, particularly towards the edges, hinting at the presence of younger, hotter stars. Faint, diffuse extensions are visible, possibly representing tidal features or ongoing interactions. There's an area towards the right which has a distinct reddish tint, potentially indicative of dust lanes or regions of older stellar populations. The absence of well-defined spiral arms indicates the galaxy is either an elliptical or a lenticular type, but its slight asymmetry suggests a prior or ongoing minor merger event may be influencing its structure.
