The galaxy presents as a slightly inclined disk. The central bulge appears prominent and exhibits a smooth, concentrated luminosity profile, suggesting an older stellar population dominating this region. Proceeding outwards from the bulge, the disk shows hints of spiral structure, though these features are not sharply defined. The overall color of the disk is somewhat bluer than the bulge, which is consistent with the presence of younger, hotter stars indicative of ongoing star formation. There is no obvious ongoing major merger or significant tidal disturbance. However, the slight irregularities in the disk's shape may suggest minor gravitational interactions in the past. Based on the overall characteristics, this galaxy could be classified as an early-type spiral or a lenticular galaxy undergoing some star formation.
