The galaxy presents as an edge-on spiral. The central bulge is prominent and appears relatively smooth and spheroidal, showing a concentrated luminosity gradient that is yellowish in color, potentially indicative of an older stellar population. The disk is visibly flattened and extends significantly outwards from the bulge, showing some mottled texture, which could suggest the presence of dust lanes or regions of active star formation. The arms are not clearly resolved. Overall, the galaxy exhibits a moderate level of star formation and an estimated stellar mass that is intermediate. There is no apparent evidence of significant tidal disturbances or ongoing mergers.
