The observed galaxy appears to be a relatively small, elongated object. The overall morphology suggests a structure that is neither perfectly spherical nor distinctly disk-like. The light distribution seems somewhat smooth, but a slight asymmetry or distortion is present, potentially indicating a past or ongoing gravitational interaction. There is a prominent blue concentration of light that is more prevalent than other areas of the galaxy. The center of the galaxy seems to be much darker than the outer edges, meaning there is likely a dust lane obscuring the light from behind. The shape of the galaxy is not perfectly round. It is not clear if this galaxy is undergoing a major merger, but there are possible gravitational disturbances.
