The galaxy presents a generally smooth, elliptical morphology. There is a centrally concentrated bulge, appearing slightly orange or reddish, which may indicate an older stellar population. Surrounding the bulge, a fainter, diffuse halo extends outwards, exhibiting a subtle blueish tint, suggesting a component of younger, bluer stars, though these may be distributed sparsely throughout the galaxy. The galaxy's overall structure suggests it is relatively undisturbed, without any major signs of ongoing mergers or tidal interactions. The light is generally even, with no clear spiral arm features. It is likely an evolved galaxy with a stellar mass that is characteristic of large galaxies. The low amount of obvious ongoing star formation suggests a low specific star formation rate. The approximate physical size suggests it is a large galaxy with a radius that can be compared to the Milky Way.
