This galaxy presents as an early-type spiral or lenticular galaxy, exhibiting a prominent bulge. The light distribution is centrally concentrated, suggesting a significant stellar population in the core region. There is a faint disk-like structure extending outwards from the bulge. The bulge appears yellowish, indicative of an older stellar population. The disk shows hints of a bluer color than the bulge, potentially indicating ongoing star formation. There is a slight asymmetry to the galaxy, possibly due to minor gravitational interaction or an internal disturbance, though no clear signs of active merging or tidal tails are present. The overall morphology suggests that the galaxy is in a relatively quiescent state, with a moderate level of star formation.
