This galaxy exhibits a slightly elliptical morphology. It presents a relatively smooth appearance, suggesting it is likely a disk galaxy viewed at an angle. The overall color profile is indicative of a lower redshift, consistent with a closer proximity. There is some evidence of faint spiral structure. The central bulge region appears somewhat subdued, indicating it may not be a dominant feature. The galaxy's light profile appears diffuse, with the highest intensity at the center. There is the presence of possible disturbance from an early merger.
