The galaxy presents as a system with a primary, brighter component and a secondary, less luminous object in close proximity. The primary galaxy exhibits a somewhat amorphous, diffuse structure with a concentrated, yellowish core region indicative of an older stellar population. A fainter, more extended halo surrounds the core, suggesting a complex stellar distribution. The secondary object appears smaller and less defined, potentially a dwarf galaxy or a tidal feature resulting from gravitational interaction. There is evidence of mild disturbance in the overall morphology, but the system does not appear to be undergoing a major merging event. The disk is not edge on. There is a small chance it is undergoing a minor disturbance due to the lower object. The system exhibits color gradients, with bluer tones in the outer regions and yellower hues concentrated towards the core, which suggests a gradient in stellar population and star formation activity across the galaxy. The size is not a large galaxy, but is not a dwarf either.
