The galaxy presents as a slightly elongated, disk-like structure with a bright central bulge. The overall color appears to be a yellow-white hue, suggesting an older stellar population within the bulge. A hint of bluer light is visible emanating from the disk, which could indicate ongoing star formation. Some irregular features are observed, suggesting the possibility of minor gravitational interactions or internal disturbances. A reddish hue is present in the more central region of the galaxy, suggesting a possible dust lane or concentration of older stars. The shape is largely smooth, but there are certain disturbances in the disk. There may be a merger occurring with the galaxy.
