The galaxy presents as a spiral structure, with two clearly defined arms visible. These arms exhibit a relatively medium winding pattern, extending outwards from the central bulge. The bulge is notable but not dominant, appearing neither overly large nor completely absent, suggesting a transitional bulge size.

The arms show evidence of active star formation regions, appearing somewhat clumpy. The overall color profile indicates ongoing star formation, contributing to the galaxy's luminosity. The spiral structure is not perfectly symmetrical, possibly hinting at past gravitational interactions or internal disturbances. Though the galaxy appears mostly isolated, there are slight irregularities on its edges. It also appears that a minor gravitational interaction could be occurring.
