The galaxy presents as a relatively smooth, elliptical structure. Its overall shape is elongated, appearing somewhat cigar-shaped, but with rounded edges that suggest a transition toward a more spheroidal morphology. A brighter, more concentrated central region indicates the presence of a galactic nucleus. The color gradient observed suggests a potentially older stellar population in the outer regions, while the inner regions have a bluer hue which may indicate some ongoing star formation. There is no obvious evidence of spiral arms or a prominent disk component. The galaxy does not exhibit any strong signs of tidal disturbances or ongoing merger activity.
