The galaxy appears to be composed of two distinct components: a more compact, centrally located region with a bright, bluish-green hue, and an elongated, less defined, and yellower extension emanating from it. The central region presents a relatively smooth appearance, lacking in clearly defined spiral arm structures. Its color suggests the presence of a relatively young stellar population and/or significant ongoing star formation.

The elongated extension has a significantly different morphology. Its yellower color indicates an older stellar population or greater dust obscuration compared to the central region. The extension is not uniformly distributed but appears somewhat clumpy, perhaps hinting at tidal interactions or recent accretion events. The overall shape of the galaxy, with its central, brighter core and extended structure, suggests a possible classification as a disturbed or interacting system.