The galaxy presents a spiral morphology, exhibiting well-defined spiral arms that originate from a bright central bulge. The spiral arms appear tightly wound closest to the bulge, becoming slightly more open as they extend outward. These arms show a mottled texture indicative of active star formation regions.

The central bulge appears somewhat prominent and spheroidal, contributing significantly to the galaxy's overall luminosity. A potential bar structure is present in the inner region of the galaxy, exhibiting elongation along the major axis.

The galaxy's disk exhibits a relatively high degree of ellipticity and is oriented at a slight angle relative to the line of sight. There is no sign of tidal tails or significant morphological distortions, suggesting a relative isolation and gravitational stability.
