This galaxy appears to be a relatively face-on spiral galaxy, with a distinct bulge and a disk component. The bulge exhibits a yellowish hue, possibly indicative of an older stellar population. The disk shows hints of bluer regions, suggesting the presence of younger, hotter stars and ongoing star formation, even if at a low rate. There seems to be a smooth distribution of light throughout the galaxy with a fairly uniform morphology. The galaxy does not appear to be undergoing any major merger events, and is likely isolated in its environment. The relatively regular morphology and lack of strong tidal features suggest the galaxy has been undisturbed for a considerable period.
