The galaxy presents as an elongated, disk-shaped structure oriented nearly edge-on relative to our line of sight. The central region exhibits a bright, concentrated bulge, appearing more yellow-white in color, suggesting an older stellar population. The disk component shows a bluer hue, potentially indicative of ongoing star formation. The disk is relatively thin and displays limited internal structure. The overall appearance suggests a lack of significant recent mergers or interactions, although subtle irregularities within the disk cannot be ruled out. The bulge appears somewhat rounded.
