The galaxy presents a distinct spiral structure. Two prominent spiral arms emanate from the central bulge, displaying a well-defined, yet somewhat flocculent morphology. The arms appear to be moderately wound.

The central bulge exhibits a substantial presence, contributing significantly to the galaxy's overall luminosity, although it isn't overly dominant. There is evidence of a bar structure within the bulge, appearing as a slightly elongated central region.

The disk component of the galaxy shows a relatively smooth texture, though some irregularities are present. The galaxy's overall shape is relatively flattened, with an elliptical appearance where the major axis is oriented roughly diagonally, and a minor axis ratio suggesting a relatively face-on view. There are no apparent signs of ongoing major mergers or significant tidal disturbances, though there are some indications of minor asymmetries in the disk that suggest minor disturbances.
