The galaxy presents as a spiral galaxy, inclined at a shallow angle to our line of sight. The central bulge is prominent and appears moderately sized, exhibiting a yellowish-white hue. A bar structure is suspected, though not strongly defined, bisecting the bulge region. Spiral arms are clearly visible, though somewhat flocculent, extending outwards from the central region, and a slight blueish tint is seen, indicating regions of active star formation. Evidence of minor disturbances exists, possibly indicative of a past or ongoing interaction with a smaller galactic object. The overall structure of the galaxy appears relatively well-defined, showing minimal signs of major merging activity.
