The galaxy presents a primarily smooth, elliptical morphology. A subtle disk-like structure might be present upon closer inspection. It's observed with an elongated shape, exhibiting an intermediate roundness. There is no evidence of a major ongoing merger, however, there appear to be some minor disturbances. The galaxy presents a central bulge and a faint, diffuse halo. There are hints of spiral arms, but they are very faint. The galaxy appears to be a relatively quiescent system with low star formation activity. The color gradient indicates that the central bulge may be older stars while the outer regions could be comparatively younger.
