The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The core exhibits a bright, somewhat unresolved, central bulge. The light gradually fades from the center outwards, suggesting a fairly uniform distribution of stars within the central region. There are hints of a more extended, fainter halo or envelope surrounding the bright core. The color appears relatively uniform across the galaxy, with a slight blueish tint. There is no strong evidence of distinct spiral arms or prominent dust lanes. The overall appearance suggests a galaxy that is relatively evolved. There are some minor asymmetries, but no strong evidence of a major ongoing merger.