The galaxy exhibits a morphology characterized by both smooth and featured components. The central region displays a predominantly smooth, bright concentration of light, suggesting a possible bulge. Extending outwards from the central region, fainter, diffuse features are observed. These features are not clearly defined as spiral arms, but rather exhibit an irregular distribution of light. There is also a small hint of a disk visible. A slight color gradient is apparent, with a bluer hue towards the outer regions. There is also an apparent disturbance in the structure of the galaxy, as if it is interacting with another galaxy, or potentially undergoing a minor merger event.
