The galaxy presents as a single system with two distinct luminous cores embedded within a common, diffuse halo. The primary core is noticeably brighter and appears slightly elongated, while the secondary core is smaller and rounder in shape. The overall light distribution is dominated by redder wavelengths, indicative of an older stellar population. There is a subtle bluish tint to the outer regions of the halo, potentially suggesting some degree of recent star formation activity. The smooth light profile suggests that the system is relatively undisturbed, despite the possible presence of multiple cores. There is no obvious spiral structure or strong tidal features, but a slight asymmetry to the halo's shape could hint at a past minor interaction.
