The galaxy presents as a spiral type, though somewhat hazy in its appearance. The spiral arms are tightly wound and appear to be quite prominent, extending from a central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. There may be a bar present based on how the spiral arms connect to the core, though not easily discernable from this image. There appears to be some minor disturbance to its morphology, but no clear signs of ongoing or recent major mergers.  There is some indication of star formation occurring, but it's not particularly vigorous. The galaxy appears relatively isolated, without any significant companion galaxies nearby that are obviously interacting. Overall, it seems to be a fairly typical spiral galaxy at a moderate distance.