The galaxy appears to be an elliptical galaxy, characterized by a relatively smooth and featureless morphology. It exhibits an elongated shape, but is largely "in between" round and cigar shaped. It presents with a central bulge that is brighter and more concentrated than its surrounding regions. There is a lack of prominent spiral arms or other distinct features typically seen in spiral galaxies. The galaxy exhibits no strong signs of recent or ongoing major merger activity, though some minor disturbances may be present. Overall, the galaxy's light profile suggests an older stellar population, consistent with limited ongoing star formation activity.
