The galaxy presents as a somewhat diffuse, elongated structure. It exhibits a noticeable blue hue, suggesting the presence of a younger stellar population and ongoing star formation. The object appears to be relatively smooth, with no clear spiral arms or distinct features immediately apparent. There is a slight flattening, giving it an oblong appearance, but this is subtle. Based on its general morphology, the galaxy may be an irregular or lenticular type, viewed close to edge-on. There is some evidence of a minor gravitational interaction or disturbance. However, this cannot be asserted with certainty from the visual data alone. Additional spectroscopic observations would be required for more accurate classification and confirmation of any potential interactions.
