The galaxy appears to be a relatively smooth, elliptical system. Its morphology is characterized by a bright, concentrated central bulge that transitions into a more diffuse halo. The galaxy exhibits a predominantly yellowish hue, indicative of an older stellar population. There is a slight bluing in the outer edges indicating some star formation. The object shows a well-defined, rounded shape, lacking any prominent tidal features or significant asymmetries that might suggest recent merger activity, though there are minor disturbances in the disk.
