The galaxy appears as a centrally concentrated object with a generally smooth morphology. It presents an elongated, disk-like structure that is not perfectly circular, exhibiting a slight deviation from roundness. The color gradient across the galaxy is subtle but noticeable, with a bluish tint towards the central regions, suggesting ongoing or recent star formation activity. Fainter yellowish hues appear in the outer regions of the galactic disk, possibly indicative of an older stellar population or dust obscuration. There are no clear signs of major disturbances in the galaxy's structure, such as tidal tails or interacting companions, although minor asymmetries might suggest mild gravitational interactions or internal processes affecting its morphology. The galaxy appears to be relatively isolated.
