The galaxy appears as a relatively small, disk-shaped structure, viewed edge-on. There is a noticeable central bulge that is more luminous than the rest of the disk. The disk itself seems relatively uniform in color, lacking prominent spiral arm structures or distinct star-forming regions. However, closer inspection suggests possible faint features or disturbances within the disk. The outer regions of the galaxy display a slightly more diffuse glow, gradually fading into the background sky. The colors of the galaxy suggest an intermediate stellar population, though the blue hue around the edge of the galaxy could indicate the presence of some younger stars, or potentially be artifactual. Possible signs of a minor gravitational interaction are present, yet the overall morphology remains generally undisturbed, lacking the classic signatures of an advanced merger event. The overall impression is that of a reasonably undisturbed disk galaxy, viewed edge-on, with a moderate amount of internal activity or disruption.
