The galaxy presents as a relatively compact object with an apparent morphology suggesting a spheroidal or elliptical shape. The light distribution appears smooth and centrally concentrated, lacking prominent spiral arm structures or a well-defined disk. The object appears nearly round. There are no obvious signs of any major merger events or tidal disturbances, though a very subtle, minor asymmetry cannot be entirely ruled out. The color appears to be generally redder in comparison to foreground objects, indicating a potentially older stellar population with less active ongoing star formation. Overall, the galaxy is consistent with an early-type galaxy at a moderate redshift.
