The observed galaxy presents as a relatively small, disk-shaped structure. It appears to be oriented approximately edge-on from our perspective. A central bulge is visible, exhibiting a noticeably brighter intensity, possibly indicative of a higher stellar density or active galactic nucleus. The disk component displays a relatively smooth appearance with minimal distinct features. There is a slight asymmetry, potentially arising from tidal interactions or internal processes. The overall color profile suggests the presence of both younger, bluer stellar populations, and older, redder populations within the galaxy. The outer regions of the disk appear somewhat disturbed, possibly indicative of ongoing or recent minor merger activity. However, a dominant, ongoing major merger is unlikely, as the galaxy's overall structure remains relatively intact. The classification suggests this object is likely a spiral galaxy undergoing some level of perturbation.
