The galaxy presents as a spiral galaxy with a relatively bright, moderately sized bulge. The disk component appears to be dominant in terms of overall size and luminosity. Distinct spiral arm structures are visible, suggesting ongoing star formation. There is no obvious bar feature present. The galaxy is not viewed edge-on. No major signs of mergers or major disturbances are observed, though minor interactions can not be ruled out. There appears to be a nearby companion galaxy in the image. The primary galaxy exhibits a blue color, indicative of a relatively young stellar population.
