The galaxy presents a generally smooth appearance, with a higher concentration of light towards the center, suggesting a bulge. There is a hint of a flattened, disk-like structure extending beyond the central region, though it is not sharply defined. The galaxy exhibits a color gradient, with the central bulge appearing more yellow, possibly indicating an older stellar population, while the outer regions show a bluer hue, suggestive of ongoing or recent star formation. There are some subtle irregularities in the outer regions of the galaxy, possibly indicating minor disturbances or interactions. Overall, the galaxy appears to be of intermediate mass, exhibiting a mix of characteristics between elliptical and spiral galaxies.
