The galaxy presents as a spiral type, observed at a moderate inclination relative to our line of sight. The central bulge region exhibits a concentrated luminosity, appearing yellow-white, indicative of an older stellar population. Prominent spiral arms are visible, displaying a grand design structure. The arms are well-defined and exhibit a two-armed morphology. The winding of the spiral arms appears to be of medium pitch, neither tightly wound nor fully open. The presence of a bar structure is suspected through the central region. The galaxy's disk shows a mottled texture, possibly suggestive of dust lanes and regions of active star formation. There is no obvious visual evidence of major mergers or significant tidal disturbances in the immediate vicinity of the galaxy, though minor disturbances cannot be ruled out. The galaxy shows a blueish hue in the arms indicating some star formation activity.