The galaxy presents as a somewhat elliptical, smooth object. The central bulge appears quite pronounced and exhibits a yellowish hue, potentially indicating an older stellar population. Moving outward from the center, the light transitions to a cooler blue color, suggesting the presence of younger, hotter stars in the outer regions. There is little evidence of distinct spiral arms or prominent dust lanes. The overall structure lacks significant irregularities or tidal features. No obvious signs of a recent major merger event are visible, though subtle disturbances may be present in the outer regions.
