The galaxy presents a dominant central bulge, appearing relatively smooth and concentrated with a yellowish hue, suggestive of an older stellar population. A fainter, bluer disk component is also visible extending from the bulge. The elongated shape suggests it is an inclined disk galaxy. The lack of prominent spiral arm structure or dust lanes indicates that it is likely an intermediate stage spiral. There are no visible signs of ongoing major mergers; however, a minor disturbance or close companion galaxy may be interacting with the primary galaxy.
