The galaxy appears to be a relatively smooth, single object. Its shape is roughly round. There is a slight color gradient, with a more yellow/red hue concentrated toward the center, suggesting an older stellar population in the core. The outer regions appear somewhat bluer. The galaxy lacks any prominent spiral arm structure or a central bar, hinting towards a more spheroidal morphology. The structure shows no significant signs of ongoing major mergers. There are some subtle indications of minor irregularities or disturbances, particularly at the edges, which could be related to either a very minor interaction, or internal disk instabilities. Overall, it presents as a relatively quiescent system.
