This galaxy presents as a moderately sized, somewhat face-on spiral, though its structure appears slightly disturbed. It has a central bulge with a yellowish hue, possibly indicating an older stellar population or the presence of dust. Surrounding the bulge is a disk-like structure displaying a mottled appearance with pockets of bluer regions suggestive of recent star formation. These regions are interspersed with areas of redder light, which could indicate older stars or dust lanes within the spiral arms. There's a subtle asymmetry to the galaxy’s overall shape, which could be the result of a past interaction or merger. A very subtle tidal tail or distortion is not overtly visible, but cannot be excluded. The galaxy exhibits a moderate luminosity, suggesting it's neither an extremely massive nor a dwarf galaxy. Its star formation rate appears subdued, indicating a galaxy that is neither actively forming stars at a high rate, nor completely quiescent. Overall, this galaxy appears to be a spiral transitioning in morphology perhaps.