The galaxy presents as a disk-shaped system, viewed at an angle of inclination that is not quite edge-on. A prominent bulge is visible, concentrated towards the galactic center, exhibiting a yellowish hue. The outer disk regions appear fainter with a bluer color, suggesting the presence of younger stellar populations and ongoing star formation. There are some subtle irregularities within the disk, potentially indicating minor gravitational disturbances or faint spiral arm structures. The overall appearance suggests a galaxy undergoing a relatively low rate of star formation, with a more substantial population of older stars in the bulge compared to the disk. There is no clear evidence of major mergers or tidal interactions.
