The galaxy appears as a relatively smooth, centrally concentrated object. The light profile suggests a spheroid-dominated morphology, characteristic of an elliptical or S0 type galaxy. There is a slight elongation present but overall, the galaxy appears nearly round. No distinct spiral arm structures are visible, nor are any prominent dust lanes or strong tidal features discernible. The galaxy exhibits a color gradient, appearing bluer towards the central region which could indicate ongoing star formation. The galaxy does not appear to be undergoing any major merging events or tidal interactions, although there are subtle irregularities in the outer isophotes that could potentially indicate a minor disturbance. The color indices indicate that the galaxy is a relatively luminous object. The galaxy does not exhibit an obvious active galactic nucleus in this view.
