The galaxy appears to be a relatively smooth and rounded system. It exhibits a concentrated central bulge with a slightly elliptical shape, surrounded by a more diffuse halo. The central region displays a redder hue, potentially indicating an older stellar population. A faint, bluish component is visible in the outer regions, which might suggest the presence of some younger, star-forming regions, but the overall star formation rate appears to be low. There is no obvious spiral structure or prominent disk, and no signs of recent or ongoing major mergers or tidal disturbances are apparent. The galaxy seems relatively undisturbed and isolated.
