The galaxy presents as an intermediate stage between a smooth elliptical and a more structured disk galaxy. There appears to be a bright central bulge, possibly indicative of an active galactic nucleus or a high concentration of stars. Surrounding the bulge, there's a fainter, more diffuse structure that suggests the presence of a disk component, although it lacks clear spiral arm definition. The overall color profile indicates a population of older stars, with a slightly redder hue in the central bulge. The outer regions of the galaxy are bluer, which might point to some ongoing or recent star formation activity. There also appears to be some degree of tidal disturbance or interaction, which leads to some asymmetry.
