The galaxy presents as a largely featureless elliptical or lenticular type. It exhibits a smooth, round morphology with a concentrated central bulge. The color profile suggests a population of older stars, leaning towards a redder spectral signature with hints of green and blue, implying a degree of ongoing, though potentially low-level, star formation. There is no obvious evidence of spiral arms or significant dust lanes. No significant signs of tidal disturbance are visible. The galaxy appears to be relatively isolated, with no clear signs of interaction or merger activity.
