The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, displaying a subtle color gradient. The core region is noticeably brighter and exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer light extends outwards from the core, hinting at possible star formation in the outer regions, although the overall star formation rate is likely low. No prominent spiral arms or other distinct morphological features are immediately apparent. There is no strong evidence of ongoing major mergers or significant tidal disturbances affecting the galaxy's overall structure, although minor disturbances are possible. The galaxy's overall color suggests a moderate redshift.
