The galaxy appears to be a relatively small, early-type galaxy, possibly an elliptical or lenticular, based on its smooth, largely featureless morphology. The light is concentrated towards the center, indicating a bright nucleus. There is a slight elongation along one axis, which is also supported by the minor merger properties. The lack of prominent spiral arms or dust lanes further suggests an older stellar population with a low star formation rate. Based on the overall color profile, the galaxy seems to be dominated by older, redder stars, though there may be some younger stars that account for the blue color.
