The galaxy presents as a relatively face-on spiral galaxy with a dominant central bulge. The core region exhibits a bright, yellowish-white color, suggesting a population of older stars. Faint, loosely defined spiral arms extend outward from the central bulge. These arms appear somewhat patchy, with subtle variations in brightness and color, indicating regions of ongoing star formation. The overall disk structure shows only a slight indication of disturbance. There is little to no evidence of a major merger event. The galaxy's color profile suggests a moderate redshift.
