The galaxy presents as a spiral galaxy with a clear central bulge that appears smooth and concentrated, exhibiting a yellowish-white hue indicative of an older stellar population.  The spiral arms are moderately defined, displaying a bluish tint, suggesting the presence of younger, hotter stars, and ongoing star formation. Dust lanes appear to be embedded within the arms. The overall shape is somewhat elongated, rather than perfectly circular and shows some minor disturbances in its morphology, suggesting the possibility of tidal interactions or a minor merger event.
