The galaxy presents as a centrally concentrated object with a relatively smooth appearance, suggesting a classification tending towards elliptical morphology, although with some characteristics of spiral morphology. The light distribution indicates a generally spheroidal shape, with an observed "in between" roundedness, but without a clear disk component or strong spiral arm features visible in this image. The galaxy exhibits a blue hue, hinting at the presence of a younger stellar population or ongoing star formation. There is a lack of any obvious major morphological disturbances or signs of a recent major merger event. There may be some minor internal disturbances.
