The galaxy appears to be a relatively small elliptical or lenticular type. It presents a smooth, concentrated central bulge, with a more diffuse, extended halo. There is little evidence of spiral arm structure, and it lacks prominent dust lanes. The core exhibits a yellow-orange hue, suggesting a population of older stars. The outer regions appear slightly bluer, potentially indicating a small amount of recent star formation or a population of younger stars. There is a slight visual disturbance to the evenness of the structure. Overall, it seems to be a galaxy with low star formation activity.
