The galaxy presents a largely smooth morphology, with minimal discernible spiral arm structure. The central region exhibits a pronounced luminosity, indicating a concentrated stellar population and possibly an active galactic nucleus, although this cannot be definitively confirmed from this image alone. The overall shape appears roughly elliptical, with a moderate degree of ellipticity. The color gradient transitions from a yellowish hue in the core to a bluer tone in the outer regions. The absence of strong tidal features or major disturbances suggests that the galaxy is relatively undisturbed. The galaxy does show some signs of minor disturbance, with a possible small merger or tidal interaction occurring.
