The galaxy appears as a centrally concentrated object with a relatively smooth, featureless morphology. It is slightly elongated, but approaches a round shape. The galaxy exhibits a dominant central bulge with a diffuse halo or disk surrounding it. The color profile is dominated by blue hues in the core, suggesting the presence of a younger stellar population or ongoing star formation. Some disturbances in its structure are present, possibly indicating a minor interaction or past merger event. The outer regions display a more mixed color composition. Overall, the galaxy presents characteristics of a transitional type, between a pure elliptical and a spiral galaxy.
