The galaxy presents as a spiral type, viewed at a moderately inclined angle to our line of sight. Two spiral arms are clearly visible, appearing tightly wound around a distinct central bulge. A pronounced bar structure appears to traverse through the central bulge, significantly influencing the spiral arm morphology. The bulge itself appears moderately sized. The disk component exhibits a bluer hue, contrasting with the yellower coloration of the bulge, suggesting ongoing star formation within the spiral arms. The galaxy appears relatively isolated with no obvious signs of major merger activity.
