The galaxy appears as a centrally concentrated, relatively smooth structure. Its morphology suggests it is likely an elliptical galaxy with a moderate size. There is a lack of defined spiral arms or prominent features typically associated with disk galaxies. The light is concentrated within its core, which could indicate an older stellar population. There may be some limited activity, but the overall impression is of a galaxy approaching quiescence. Any merging activity in the recent past seems unlikely due to the galaxy's regular appearance.
