The galaxy presents as a somewhat elongated, disk-like structure, oriented at an angle to our line of sight. The central bulge appears bright and yellowish, indicative of an older stellar population. Fainter, bluer regions are visible in the outer disk, potentially suggesting ongoing star formation. The galaxy does not exhibit a clear spiral arm structure or any signs of strong tidal disturbances. The overall morphology suggests a relatively quiescent galaxy, possibly a late-type spiral or a lenticular galaxy with a moderate amount of star formation activity.
