The galaxy presents as a somewhat elliptical, disc-like structure with a concentrated central bulge that is yellowish-white in color, suggesting an older stellar population. There are suggestions of faint spiral arms or extensions extending outwards. The outer regions are more diffuse and appear bluer than the central bulge, implying the presence of younger stars or active star forming regions. There is a hint of a disc component, although this could be a result of viewing angle. There are no clear signs of significant recent merging activity or major tidal disturbances.
