The galaxy presents a generally smooth morphology, appearing elliptical in shape. Its central region exhibits a pronounced concentration of light, with a color profile trending towards redder wavelengths. This core is surrounded by a more diffuse halo, where bluer colors are apparent, potentially indicating the presence of a younger stellar population. The halo lacks distinct features such as spiral arms or prominent dust lanes, lending further credence to its classification as an elliptical or lenticular galaxy. There is no evidence of active galactic nuclei or significant ongoing star formation within this galaxy. The galaxy is slightly elongated. No other galaxies seem to be visibly merging with it, or causing any disturbances.