This galaxy appears to be a relatively smooth, disk-shaped object, likely a spiral or lenticular type seen edge-on. Its central bulge exhibits a yellowish hue, suggesting a population of older, redder stars. The disk component, extending outwards from the bulge, has a slightly bluer color, implying ongoing star formation, though at a seemingly low rate. The galaxy's morphology is mostly undisturbed, with no obvious signs of a major merger or significant tidal disruption. It does show a slight cigar shape, being more extended than round. There might be some minor disturbances internally within the galaxy, but it appears to be primarily an isolated system. 
