The galaxy appears as a somewhat diffuse object with a subtle, disk-like morphology. There's a slight concentration of light towards the center, suggesting a possible bulge component, but it's not sharply defined. The overall color is a moderately red hue, which implies a population of older stars and potentially a lower rate of ongoing star formation. There are hints of some faint, bluer regions embedded within the galaxy's disk, possibly indicating areas of more recent star formation, although these regions are not very prominent. There is no evidence of strong spiral arm structures or a bar. The galaxy doesn't appear to be undergoing a major merging event, although there may be some minor tidal features or asymmetries hinting at past interactions or minor disturbances. Overall, the galaxy presents a relatively smooth, quiescent appearance.
