The galaxy presents as a spiral, although the disk appears somewhat disturbed. Faint spiral arm structures can be discerned. The central bulge is prominent, moderate in size, and exhibits a yellowish-orange hue. Overall, the galaxy's color suggests a mixture of stellar populations with a significant contribution from older, redder stars. Some of the disk appears to be disrupted or irregular, possibly due to interactions or recent star formation. There are few defined star forming regions within the arms. The majority of the color seems to be a yellow hue. There is no obvious bar structure visible from this view.
