The galaxy presents as a moderately luminous, centrally concentrated elliptical type. It exhibits a generally smooth morphology with a noticeable lack of distinct spiral arm structures or prominent dust lanes. The overall shape is somewhat elongated, deviating from a perfectly circular form. A colour gradient can be observed, with the central region appearing more yellow/orange, suggesting an older stellar population. Fainter, bluer outskirts are present, implying the presence of a younger stellar population or potentially ongoing, albeit minimal, star formation. No obvious signs of major mergers or tidal disturbances are apparent, although a minor asymmetry cannot be ruled out at this resolution.
