This galaxy presents as a disk galaxy, viewed at an approximate edge-on orientation relative to our line of sight. A central bulge is discernible, exhibiting a yellowish hue, indicative of an older stellar population. The galactic disk appears as a flattened structure extending outwards from the bulge. Dust lanes are faintly visible within the disk, obscuring some of the starlight and contributing to the overall reddish color. There is no apparent ongoing major merger event, although subtle asymmetries in the disk may suggest minor gravitational interactions or disturbances. The lack of prominent blue regions or HII regions implies a relatively low rate of recent star formation.
