The galaxy presents as a spiral type with a moderately sized bulge. Two prominent spiral arms emanate from the central region, exhibiting a relatively medium winding. Star formation appears active within these arms, indicated by their bluer hue in comparison to the yellowish bulge. The disk component is dominant. No major disturbances are apparent, though the image suggests a slight asymmetry in the spiral structure, possibly indicative of a past minor interaction. The arms display a complex structure, hinting at ongoing star formation regions. The general morphology suggests a galaxy that is neither excessively young nor particularly old, but rather one in a phase of sustained star formation.
