The galaxy appears to be a relatively compact, elliptical or lenticular galaxy. It exhibits a smooth, centrally concentrated light profile with a noticeable lack of spiral arm structures or significant dust lanes. The galaxy's color suggests an older stellar population, with a subtle reddish hue overall, implying a lack of substantial ongoing star formation. The morphological classification, based on visual inspection, leans towards a largely undisturbed system without major signs of tidal interactions or mergers. It displays a general roundness, neither extremely flattened nor cigar-shaped. There's no obvious evidence of a prominent disk component, although a faint flattened structure can't be entirely ruled out. The galaxy shows a relatively high luminosity with a considerable mass content.
