The object presents as a compact galaxy, approximately circular in projection with a slight elongation observed in the vertical direction. The galaxy exhibits a distinct color gradient, with a bright, cyan core suggesting a high concentration of ionized gas and ongoing star formation. Surrounding the core is a fainter, diffuse halo, with a predominantly green hue, indicating a population of older stars. There is faint hint of a faint blue region above the core. The central region is notably smooth in appearance, lacking any obvious spiral arm structures or dust lanes. Based on these observations, the galaxy is likely an elliptical or lenticular galaxy with possible signs of recent or ongoing merger activity. Minor disturbances are present at the bottom of the galaxy, indicating a possible recent or ongoing merger. 
