This galaxy presents as a generally smooth, centrally concentrated object. Its shape is close to round, with only a slight deviation towards an elliptical form. There are no obvious spiral arms or a distinct disk component visible. The color profile suggests a relatively older stellar population, with a lack of prominent blue star-forming regions. There are hints of possible disturbances in the galaxy’s structure, perhaps indicating past or ongoing minor interaction with another galaxy. The overall impression is of a galaxy that is transitioning away from an active star-forming phase, possibly evolving towards a more quiescent state.
