The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that is bright and appears yellow-orange in color. The outer regions of the galaxy fade gradually into the background, suggesting a less dense stellar population. The galaxy's shape deviates slightly from perfectly circular, appearing somewhat elongated. There is no apparent spiral structure or prominent dust lanes. The overall color suggests an older stellar population with reduced ongoing star formation. The absence of significant distortions in its shape suggests the galaxy has not undergone a major merger event recently, though a minor interaction cannot be ruled out based on this image alone.
