The galaxy presents as a centrally concentrated object with a relatively smooth light profile. The core displays a yellow-orange hue, suggestive of an older stellar population. There is an extended, fainter, blueish halo surrounding the central region, potentially indicating more recent star formation activity within the galactic disk or tidal debris. Evidence of possible merger activity or tidal interaction can be seen via minor morphological disturbance, with the core appearing to have two additional areas of higher density surrounding it, suggesting a recent or on going merging event. The galaxy exhibits an approximate redshift of 0.233, indicating a substantial cosmological distance and lookback time.
