The galaxy presents as a relatively smooth and concentrated object. It exhibits an elliptical morphology, appearing somewhat rounded but not perfectly spherical. The central region displays a yellowish hue, indicative of an older stellar population. Moving outward from the core, a gradual transition towards a bluish tint is observed, possibly suggesting the presence of younger, hotter stars in the outer regions or a lower metallicity. There's no clear evidence of spiral arms or a distinct disk structure; any such features are either absent or obscured due to the galaxy's distance and/or viewing angle. There appears to be a subtle asymmetry to the galaxy’s outer contours, with a slight elongation along one axis. No significant signs of ongoing major mergers or strong tidal disturbances are visible.
