The galaxy presents as a generally smooth object, with a distinct central bulge that graduates into a more diffuse disk. The galaxy's shape is elongated, tending towards a cigar shape, with a high degree of roundness in its light profile. There is no indication of strong spiral arm structures or major mergers. The galaxy appears to be relatively isolated, exhibiting no significant tidal disturbances or interactions with nearby galaxies. The colour gradient moves from a bright, slightly yellow-white center to a bluer halo, which may indicate a difference in star formation rates or stellar populations between the central and outer regions.
