The galaxy presents a generally smooth morphology, appearing somewhat elliptical or spheroidal in shape. There is an evident central bulge, which exhibits a brighter, more concentrated luminosity compared to the outer regions. A slight color gradient is observed, with the central region displaying a warmer hue, possibly indicative of an older stellar population or dust obscuration. The outer regions exhibit a bluer tint suggesting the presence of some younger stars. The lack of clearly defined spiral arms or a prominent disk structure reinforces the classification as a relatively smooth system. There may be some minor disturbances or early stages of merging activity given the asymmetrical distribution of light in the outer regions.
