The galaxy presents as a somewhat elongated, disk-like structure, with an apparent inclination relative to our line of sight. A bright central bulge is evident, exhibiting a yellowish-white hue suggesting a population of older stars. Fainter, bluer features extend outward from the bulge, potentially indicative of more recent star formation activity within the spiral arms. The overall appearance is relatively smooth, with no distinct, bright knots or regions of intense star formation readily apparent in this image. There are signs of faint dust lanes within the disk. There are also potential signs of minor tidal interactions in this image.