The galaxy presents as an elliptical morphology, lacking any obvious spiral arm structure. Its overall color appears yellowish-white, suggesting an older stellar population. The light is centrally concentrated with a smooth and gradual decrease in luminosity moving outwards from the core. There is minimal evidence of dust lanes or significant regions of recent star formation, with only a few very faint blue regions surrounding the central bulge. These regions are faint which could suggest there is ongoing star formation at a low rate. The outer regions of the galaxy appear diffuse and poorly defined, lacking any sharp boundaries, which is consistent with an elliptical galaxy. The galaxy does not appear to be undergoing any major mergers or exhibiting strong tidal distortions, but there is minimal evidence that could suggest there is a minor interaction occurring.
