The galaxy presents an overall elliptical morphology, appearing elongated along a discernible axis. The central region exhibits a bright, concentrated core, suggestive of a significant stellar population and potentially a supermassive black hole. A diffuse halo surrounds the core, fading gradually into the background.

A distinct dust lane bisects the galaxy, oriented approximately perpendicular to the major axis. This lane appears as a dark, reddish-brown band, indicating the presence of obscuring material. The dust lane is not uniformly distributed, displaying some clumpy structures within it.

The overall color gradient transitions from a bluer hue in the central region to a redder tone in the outer parts. This may indicate a younger stellar population in the core, while the outer regions are dominated by older, redder stars. There are some subtle indications of possible tidal distortions or interactions, which should be analyzed with a deeper inspection of the surrounding area.
