The galaxy presents as a single, relatively smooth, and rounded object. The light profile is somewhat centrally concentrated, appearing brightest toward the core. The color of the galaxy is generally yellowish, suggesting an older stellar population. There is a faint object possibly in the process of merging. No obvious spiral arm structures or prominent dust lanes are discernible. It does not show signs of significant recent star formation. The morphological analysis suggests the galaxy is not currently undergoing a major merger.