The galaxy presents as a centrally concentrated, luminous object, exhibiting a smooth, elliptical morphology. The core displays a yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, the galaxy transitions into a more diffuse, fainter region with subtle blue-ish tinges. This suggests a trace amount of ongoing or recent star formation. No distinct spiral arms or bar structures are discernible, consistent with a galaxy dominated by a spheroid component. There are very slight disturbances visible in the galaxy's structure. Overall, it appears to be a moderately massive galaxy at an approximate redshift of 0.27.
