The galaxy presents as a spiral type, although the spiral arms are not sharply defined. There is a substantial central bulge, occupying a considerable fraction of the galaxy's total area and exhibiting a smooth, yellowish hue suggestive of an older stellar population. A bar structure is present across the center, moderately prominent. Surrounding the bulge, the disk appears somewhat patchy and flocculent. There are hints of spiral structure, but the arms are not continuous or well-defined; they seem more like fragmented segments. Overall the galaxy has more of a yellow/red hue. No merging is apparent based on the morphology of the galaxy. The inclination is a face on view.
