The galaxy presents a largely smooth morphology, with a high probability of it being elliptical. The central bulge is prominent and appears relatively spherical, dominating the overall light distribution. There is a clear concentration of light toward the center, indicating a dense core. While mostly smooth, there might be subtle features hinting at a very faint disk-like structure in its periphery, although this is difficult to confirm due to its low prominence. There appear to be no signs of ongoing major mergers or significant tidal disturbances, with only a hint of some minor disturbances. Its general appearance suggests an evolved system with a comparatively low rate of star formation. The overall color is moderately red, consistent with an older stellar population and low dust content. The galaxy appears relatively isolated.
