This galaxy presents as a slightly inclined, disk-shaped system. The central bulge appears prominent and exhibits a yellowish hue, possibly indicative of an older stellar population. The disk component shows evidence of spiral arm structure, although these features are somewhat diffuse and lack high resolution. The outer regions of the disk display a bluer color, potentially suggesting ongoing star formation within these areas. There is no apparent presence of a strong bar or ring structure. The galaxy appears relatively isolated, with no obvious signs of recent or ongoing merger activity. Overall, it exhibits characteristics consistent with a late-type spiral galaxy, possibly an Sc or Sd type, viewed at a moderate inclination.
