The galaxy appears to be a relatively bright, disk-shaped system with an apparent intermediate inclination to our line of sight. It exhibits a prominent central bulge that is more luminous and displays a yellowish-white color, suggesting an older stellar population. Fainter, bluer light is present in the outer disk region. There are possible signs of a faint spiral arm structure present at the outer edges of the galaxy, but the image resolution makes it difficult to confirm. The overall color index suggests a system with ongoing, albeit relatively moderate, star formation. There are no obvious signs of strong tidal interactions or major disturbances, though some minor asymmetry in the outer disk could potentially indicate a past or ongoing minor merger event. The galaxy presents a generally smooth appearance, with no extremely bright or distinct star-forming regions immediately apparent. The elongated shape indicates it is not a face-on spiral galaxy, but rather is tilted somewhat relative to our perspective.
