The galaxy presents as a slightly inclined disk galaxy. The central bulge is prominent, appearing with a yellowish hue, suggesting a population of older, redder stars. The disk appears moderately well-defined, with subtle hints of spiral arm structure. The arms are somewhat flocculent. There are hints of bluer regions in the disk, potentially indicating areas of ongoing star formation, especially in some of the spiral arm regions. Overall, the galaxy exhibits a relatively smooth appearance with some signs of a possible minor disturbance.
