The galaxy presents a generally smooth morphology, suggesting an early-type classification. The light distribution is centrally concentrated with a diffuse, extended halo. The central bulge exhibits a yellowish-white color, potentially indicative of an older stellar population. Faint blue hues appear in a patchy, indistinct disk or outer region, hinting at ongoing, but modest, star formation activity. The overall shape approximates a slightly elongated ellipse. There is no evidence of major tidal disturbances or ongoing mergers based on the galaxy's structure. Subtle, minor irregularities might be present in the outer regions.
