The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. It appears to have a dominant bulge component with a gradual decrease in luminosity outwards. No distinct spiral arm structures or prominent dust lanes are discernible in this image. There is a subtle color gradient, shifting towards bluer hues in the outer regions, suggesting the presence of younger stellar populations compared to the core. The overall color indices indicate that the galaxy's stellar population is composed of both old and young stars. There is no indication of any major mergers or significant tidal disturbances affecting the galaxy's overall structure, although there is a hint of a minor irregularity in the morphology.
