The galaxy presents as a smooth, elongated elliptical form, suggesting an older stellar population. It exhibits a yellowish hue, indicating a lack of significant ongoing star formation and a dominance of older, redder stars. The galaxy appears relatively undisturbed, lacking prominent spiral arms, bars, or other features indicative of recent mergers or interactions, though there is a slight disturbance in its otherwise smooth morphology. Its moderate redshift suggests that it is a relatively distant object. The overall appearance indicates a galaxy with a substantial stellar mass and a relatively low specific star formation rate.
