The galaxy presents as a relatively smooth, centrally concentrated structure. Its morphology appears to be largely spheroidal with a dominant bulge. The light profile suggests a high degree of central concentration with an overall elliptical shape. The galaxy exhibits a yellow-reddish hue, possibly indicative of an older stellar population with ongoing, but suppressed, star formation. There is very little evidence of a disk component or spiral arm structures. The smooth appearance suggests a lack of recent major mergers, although some minor gravitational disturbances may be present.
