The galaxy presents as an elliptical or lenticular structure with a relatively smooth, featureless appearance. It displays a centrally concentrated bulge that dominates the overall luminosity profile. There is a discernible color gradient, with the core exhibiting a yellowish-orange hue that transitions to a redder color in the outer regions, suggesting an older stellar population toward the outskirts. The absence of prominent spiral arms or distinct dust lanes implies a lack of significant ongoing star formation. The galaxy appears largely undisturbed, without any obvious signs of tidal interactions or recent merger events. The overall shape is moderately elliptical, exhibiting a slight deviation from perfect circularity.
