The galaxy presents as a slightly elongated, disk-like structure seen at a moderate inclination. It has a smooth appearance, with a high degree of central concentration. The core appears bright and yellowish, possibly indicative of an older stellar population dominating the central region. Extending outwards from the core is a fainter, bluer disk. There is a hint of subtle disturbances, perhaps minor tidal interactions, but no significant merger events are visibly distorting its overall shape. The galaxy exhibits intermediate roundness. The slight color variation across the galaxy suggests ongoing, but not extreme, star formation.
