The galaxy appears to be a relatively face-on spiral galaxy, exhibiting a degree of smoothness. The central bulge is prominent and has a yellowish hue, suggesting a population of older stars. Surrounding the bulge is a fainter, more diffuse disk component. There are hints of spiral arm structure within the disk, although it's not sharply defined. Some regions within the disk appear slightly bluer, potentially indicating areas of ongoing star formation. The galaxy's overall shape is somewhat rounded, leaning towards elliptical. There is no evidence of major mergers or significant tidal disturbances, suggesting the galaxy has been relatively undisturbed.
