The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, centrally concentrated light distribution. It presents an overall yellowish hue, suggestive of an older stellar population with a relative lack of ongoing star formation. The galaxy exhibits a moderate degree of roundness, not appearing overly flattened or elongated, but instead approaching a spheroidal shape. There are no readily discernible tidal features, strong distortions, or other clear signs of recent major merger activity. Faint color gradients may be present within the galaxy, potentially indicating subtle variations in the age or metallicity of the stellar populations across the galaxy’s extent.
