The galaxy presents as a central, somewhat concentrated bulge region surrounded by a fainter, more diffuse disk. The bulge exhibits a slightly elongated, rather than perfectly spherical, appearance. There is limited evidence of spiral arm structure, rather the disk appears smoother in texture. The galaxy has an overall bluish hue, suggesting the presence of some younger stellar populations within the observed spectral range. There are minor irregularities present in the outer regions, but no conclusive indications of tidal streams or major mergers. A very slight degree of asymmetry is present in the outer disk, indicating potentially minor interactions in its past.
