The galaxy presents as a spiral type, viewed at a moderate inclination, not quite face-on but not fully edge-on either. Two distinct spiral arms are observable emanating from a central bulge region. The arms exhibit a relatively open winding pattern, neither tightly wound nor extremely loose. The bulge appears moderate in size, contributing a significant portion to the galaxy's overall luminosity. A bar structure is present, extending from the central bulge and influencing the morphology of the spiral arms. Star formation appears active within the spiral arms, indicated by the presence of bluer regions suggesting younger stellar populations. No major distortions or tidal features are apparent, suggesting the galaxy is not currently undergoing a major merger event, though some minor disturbance cannot be ruled out. The overall color profile suggests a mix of stellar populations, with both younger, bluer stars in the arms and older, redder stars concentrated in the bulge.
