The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. There appears to be a dominant bulge component, exhibiting a yellowish-white color, suggesting a population of older stars. The disk is faintly visible but lacks distinct spiral arm structures; it seems relatively smooth and blended with the bulge. The outer regions of the galaxy show a gradual decrease in luminosity, fading into the background sky. There is little evidence of strong star formation activity based on color; no prominent blue regions or HII regions are observed. The overall morphology suggests the galaxy may be an early-type spiral or a lenticular galaxy, possibly undergoing little to no major merging events. The image doesn't reveal any pronounced tidal features or strong signs of gravitational disturbance.
