The galaxy presents as a spiral type, observed at an angle slightly inclined from face-on. A central bulge is visible, exhibiting a concentrated luminosity with a yellow-orange hue, suggesting an older stellar population. Extending outwards are two prominent spiral arms, tracing a grand-design pattern. The spiral arms show indications of active star formation regions, exhibiting a bluer color.

The overall structure appears relatively well-defined, though some irregularities suggest possible past minor gravitational interactions or internal disturbances. The galaxy does not obviously show any strong bar structure. It also does not seem to be undergoing any major merging activity.
