The galaxy appears to be a disk galaxy, seen at an inclined angle. The central bulge exhibits a yellowish hue, indicative of an older stellar population. The disk component displays a bluer tint, suggesting ongoing star formation. Faint, somewhat disrupted spiral arms are present, implying potential interactions or disturbances. The overall morphology suggests a galaxy that is neither perfectly elliptical nor a grand-design spiral, but somewhere in between. The galaxy exhibits a relatively smooth, slightly elongated structure.
