The galaxy presents an elliptical morphology, exhibiting a smooth, diffuse light distribution across its structure. There is a noticeable central bulge, appearing bright and concentrated. The overall color suggests an older stellar population, with a yellowish hue dominating. Hints of a faint, flattened disk component are visible along the equatorial plane. A slight asymmetry in the outer regions may indicate a past or ongoing minor interaction. The galaxy appears relatively isolated in the field of view, with no obvious signs of a major merger event.
