The galaxy appears to be a luminous, yellowish elliptical. It exhibits a smooth morphology, lacking discernible spiral arms or a prominent disk structure. The light is centrally concentrated, indicative of a substantial bulge component. The galaxy seems generally undisturbed, without obvious signs of recent major mergers or tidal interactions, although a slight asymmetry and a faint possible distortion on one side could be indicative of a minor interaction. The round shape indicates that it is most likely an E0-E3 galaxy. The color suggests a population of older stars and a relatively low rate of ongoing star formation. Its estimated size is substantial, suggesting it is a reasonably massive galaxy.
