The galaxy presents as an elliptical structure with a smooth, centrally concentrated bulge. There is a subtle disk component, showing minor features of possible spiral arms. The central bulge appears to have a yellow-orange hue, suggesting an older stellar population. Fainter, bluer light is visible in the outer regions of the disk, potentially indicating ongoing star formation. The galaxy’s overall shape is elongated, displaying a slight cigar-like morphology. There are no obvious signs of a major merger event, but some minor disturbance cannot be ruled out.
