The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a round appearance, presenting as nearly circular on the plane of observation. The core is intensely luminous, with the intensity decreasing significantly towards the edges. There is no discernible spiral structure or bar feature. Minimal evidence of tidal interactions or mergers is present, with no obvious asymmetric features, extended tidal tails, or other signs of recent gravitational disturbance. The galaxy shows a prominent redder color as observed through the r and z bands, suggesting a population of older stars. Overall, the galaxy appears to be an elliptical galaxy or a lenticular galaxy with limited ongoing star formation.
