The galaxy presents as a disk-shaped structure, with a pronounced central bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population. The disk is oriented approximately edge-on relative to our line of sight, with its major axis running horizontally across the image. Faint blue tinges are visible within the disk, hinting at the presence of younger, hotter stars, potentially indicative of ongoing star formation. There are some visual hints of spiral arm structure. The outer edges of the galaxy appear somewhat irregular, suggesting possible past interactions or mergers, though no major disturbances are apparent. The galaxy is moderately luminous with an estimated stellar mass on the order of 10^10 solar masses and moderate levels of star formation activity.
