The galaxy presents as a roughly elliptical object. There is a central, concentrated bulge region exhibiting a yellowish hue, suggesting a population of older stars. Surrounding this bulge is a more diffuse, bluish halo. The blue color suggests the presence of younger, hotter stars and potentially ongoing star formation in these outer regions. The morphology appears relatively undisturbed with no clear signs of a major merger event. Some minor irregularities or faint features may be present in the outer halo, possibly indicating minor disturbances or tidal interactions. Overall, the galaxy seems to be an intermediate-mass system with a mix of stellar populations and moderate levels of star formation activity.
