The galaxy presents as a spiral type, viewed at an oblique angle. The overall structure appears asymmetric, suggesting possible gravitational interaction or past merger events. Two prominent spiral arms are discernible, exhibiting a loose winding pattern. Star formation appears distributed throughout the arms, with some indication of HII regions within the spiral arms. The central bulge is relatively small, with a smooth morphology and an yellowish hue, indicating a population of older stars and low star formation. No strong bar structure is apparent. Faint tidal features or distortions are observed, possibly resulting from a past or ongoing interaction. The galaxy appears relatively isolated with no other galaxies nearby.
