The galaxy presents as a disk-shaped structure, observed edge-on relative to our line of sight. There appears to be a central bulge, though it is not very prominent. There is a low degree of internal structure discernible, although a slight unevenness in the light distribution may hint at some faint spiral arms or dust lanes. The color gradient suggests a degree of ongoing star formation, with a bluer hue toward the outer edges and a redder hue toward the central bulge, indicative of older stellar populations concentrated in the core. The overall shape of the galaxy appears relatively undisturbed, with no significant tidal features or distortions apparent, suggesting it is not currently undergoing a major merger event.
