This galaxy presents as a spiral type, although the inclination obscures a clear view of the arm structure. The nucleus is bright and concentrated, surrounded by a slightly elongated bulge. The disk appears relatively smooth with hints of bluer regions, potentially indicating areas of ongoing star formation. The overall color index suggests a mix of older stellar populations in the bulge and younger, bluer stars in the disk. The galaxy doesn't show signs of significant tidal distortion or ongoing mergers, but some minor disturbances within the disk cannot be ruled out at this resolution. The presence of spiral arms seems likely based on subtle features, though an accurate count or characterization is difficult.
