The galaxy presents as a centrally concentrated object, exhibiting a mostly smooth morphology, with some faint indications of a disk like structure. The light distribution suggests a possible elliptical galaxy, though not perfectly spherical, leaning more towards an oblate spheroid. The central region exhibits a bright, yellowish hue, potentially indicative of an older stellar population or active galactic nucleus. Fainter, bluish colors extend outwards from the core, possibly indicating some younger star formation. There is a mild asymmetry within the galaxy. No strong signs of recent major merger events, or tidal tails are visible.
