The galaxy presents as a relatively smooth, elliptical-like structure. Its light is dominated by a yellowish hue, which is highly concentrated in its central region, suggesting an older stellar population and a lack of significant ongoing star formation. There is a very subtle flattening of the galaxy’s morphology, shifting it slightly from perfectly round towards a more elongated, cigar-like shape.

There are no obvious signs of spiral arms or dust lanes. The galaxy appears isolated, with no immediately apparent tidal features or close companions indicating a recent major merger event, although subtle asymmetries may be present. The overall smooth appearance suggests a well-mixed stellar population and a lack of significant recent disturbances. The galaxy appears to be a relatively massive system with a high degree of stability.
