The galaxy presents as an elliptical form with a smooth, largely featureless morphology. The central region exhibits a concentration of light, appearing a yellowish-orange hue, suggestive of an older stellar population. Moving outward from the core, the galaxy fades into a more diffuse, bluish halo. The overall shape suggests a spheroid, but with a moderate elongation, verging towards a cigar shape. There is no clear evidence of significant ongoing merger activity or major disturbances in its structure, although a subtle asymmetry might indicate a minor interaction in its past. Faint blue tinges at the edges might suggest some low level star formation in cooler regions. Based on its color profile, the galaxy likely has a substantial mass and a modest ongoing rate of star formation.
