The object is a lenticular-like galaxy exhibiting a moderately inclined disk. The galactic nucleus presents a bright, concentrated bulge, suggesting a significant population of older stars. The disk component appears relatively smooth and featureless, lacking prominent spiral arm structures. The overall color profile appears to be on the bluer end, perhaps indicating the presence of younger stars, although this is not immediately apparent from any star forming regions. There may be some slight asymmetry or faint tidal features present, suggesting a possible minor gravitational interaction in its past.
