The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its core exhibits a bright, yellowish-white hue, suggestive of an older stellar population dominating the central regions. The light tapers off gradually from the core, indicating a lack of strong, defined spiral arms or a prominent disk structure. There are subtle color variations observed in the outskirts of the galaxy, transitioning towards a more reddish tint, hinting at potentially older or dustier regions further from the galactic center. There is a second, orange-colored object that could possibly be tidal debris, or a star cluster, but this association is uncertain. Overall, the galaxy's appearance aligns with that of an elliptical or lenticular galaxy at a moderate redshift, displaying a relatively quiescent state of star formation, though there appears to be a low level of ongoing or recent star formation activity. The galaxy does not appear to be undergoing any major merging events, though subtle disturbances cannot be ruled out based on the image alone.
