The galaxy presents an overall smooth morphology. There is a concentrated central bulge, appearing with a yellow-orange hue, suggesting an older stellar population. The surrounding disk, if present, lacks distinct spiral arm structure. The shape is somewhere between round and elongated, but appears mostly round. There is a slight suggestion of minor gravitational disturbance in the outer regions. No obvious tidal tails or significant morphological irregularities indicative of a major merger are apparent. The galaxy exhibits a gradual color gradient from the core to the outer regions, with the core exhibiting a yellower color, and the outskirts showing a subtle shift towards blue, this could be due to differential stellar populations. The object shows no definitive signs of active galactic nuclei activity based on its visual appearance, no bright jets or ionized gas. The object presents itself as relatively undisturbed.
