The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology with a generally rounded shape. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The color profile indicates a dominant population of older stars, contributing to a reddish-yellow hue in the central region. There is no evidence of spiral arms or a prominent disk structure. No signs of tidal tails or other major disturbances are visible, suggesting it has not undergone a major merger in recent history. Faint blue stars are scattered through the outskirts of the galaxy. Overall, the galaxy presents a passively evolving system.
