The galaxy presents as a luminous, disk-shaped structure oriented at an oblique angle to our line of sight. The central bulge is prominent and appears relatively smooth and featureless, indicating a significant population of older stars. The disk exhibits a fainter, more diffuse glow extending outwards from the central region. There is some indication of spiral arm structure, though the arms are not well-defined and are likely tightly wound. The overall color profile suggests a relatively mature galaxy with ongoing, but not exceptionally high, star formation. There is a slight asymmetry to the outer regions of the disk, possibly indicative of minor tidal interactions or past merger events. The galaxy's shape appears to be somewhere between elliptical and a cigar shape. There does not appear to be any major ongoing mergers occuring with this galaxy.
