The galaxy appears to be a disk galaxy, viewed at a moderate inclination. A central bulge is visible, appearing bright and relatively smooth. Faint spiral arms are visible emanating from the central bulge, though they lack significant structure. The galaxy's color suggests a mix of stellar populations, with a bluer hue in the disk potentially indicating ongoing star formation. There may be some interaction or minor disturbance within the galaxy, indicated by the overall shape, but this could also be a result of the moderate inclination. It is likely that the galaxy is not currently undergoing a major merging event, or that the merger is in its late stages where there is no significant change to its physical structure. 
