This galaxy appears to be a relatively small, disk-shaped system observed at a significant inclination to our line of sight. A central bulge is visible, appearing somewhat concentrated and bright. The disk component displays a mottled texture, potentially indicating the presence of spiral arms or irregular star-forming regions. There are hints of dust lanes within the disk, obscuring some of the starlight. The overall color suggests a mix of stellar populations, with a somewhat redder color in the bulge region compared to the disk, perhaps indicating older stars in the center. There is a slight asymmetry to the disk, which may suggest some kind of gravitational disturbance.
