The galaxy presents a generally smooth, rounded morphology. The light distribution exhibits a concentration towards the central region, with a gradual decline in luminosity outwards. There is an absence of discernible spiral arms or a well-defined disk structure, although a slight flattening may be inferred. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or significant tidal interactions. The central bulge displays a yellowish hue, which could indicate an older stellar population or a higher concentration of dust. The overall color suggests an intermediate type. Evidence of ongoing star formation appears to be minimal.
