The galaxy exhibits a flattened, elongated morphology, suggesting it is likely a disk galaxy viewed at an oblique angle. The central region appears brighter and more concentrated, indicating the presence of a galactic bulge. A slight color gradient is noticeable across the galaxy, transitioning from a more yellow/red hue in the central bulge area to a slightly bluer tint in the outer disk. This could indicate younger star formation in the outer regions. The overall structure appears relatively smooth, with little evidence of prominent spiral arms or other distinct features. There is a hint of minor disturbance or asymmetry, which could be due to a past or ongoing interaction with another galaxy, but it seems overall unperturbed. Based on these features, I estimate that this galaxy is a moderately sized spiral galaxy viewed at an angle, potentially undergoing some level of star formation in the disc.
