The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical, exhibiting a generally round shape. There is no obvious disk structure or spiral arm morphology visible. Light from the core is concentrated, with a gradual fall-off in luminosity towards the outer regions of the galaxy. Subtle hints of irregularities suggest minor disturbances in the morphology. There are no obvious signs of ongoing major merging events, although some minor interaction may be occurring. The overall color profile is yellowish, consistent with an older stellar population, and relatively low levels of star formation.
