The galaxy presents as a spiral type, viewed at a significant inclination, appearing nearly edge-on. Its disk structure is prominent.

The central bulge is moderately sized relative to the overall dimensions of the galaxy, exhibiting a yellowish hue indicating an older stellar population. Faint spiral arms are observable extending outwards, though the resolution limits a detailed tracing of their morphology. There is some evidence of a faint bar-like structure transecting the central bulge along the major axis of the galaxy.

The overall color profile shows a trend from yellow/white in the central regions to bluish hues in the outer arms. The presence of bluer regions in the arms suggests regions of active star formation. The galaxy exhibits no obvious signs of any ongoing major mergers or significant tidal disturbances.
