The galaxy presents as a somewhat elliptical structure with a bright, concentrated central region. This suggests the presence of a substantial galactic nucleus. A disc structure is subtly visible, displaying relatively smooth features. There is a slight disturbance in one of the arms, which may be indicative of ongoing minor gravitational interactions. The overall color profile appears slightly redder, suggesting an older stellar population, but some bluer regions can be seen, potentially indicating a modest amount of on-going star formation.
