The galaxy appears as a disk galaxy, seen nearly edge-on. The central bulge is prominent, exhibiting a yellowish-white hue suggestive of an older stellar population. This bulge appears relatively smooth and concentrated. A thin disk extends outward from the bulge, with a fainter blueish tint. The overall morphology indicates little to no significant interaction with other galaxies, presenting a relatively undisturbed structure. Star formation seems to be present within the disk, but not at an extremely high rate. The disk's uniformity suggests a well-established and stable galactic structure, with limited evidence of ongoing major mergers or disruptive events.
