The galaxy appears to be an irregular or possibly disturbed spiral galaxy, with an estimated effective radius around 6 kpc. Its overall morphology suggests a system that may be undergoing or has recently undergone a merger or significant interaction, indicated by the presence of faint tidal features and disturbed disk. The color indices, derived from DESI g, r, and z band magnitudes, suggest a relatively older stellar population with some ongoing star formation. The low specific star formation rate indicates that the galaxy is not experiencing a major starburst. The galaxy's stellar mass is substantial, placing it within the range of massive galaxies at its redshift. The light distribution is somewhat clumpy, possibly due to recent or ongoing star formation or tidal debris from the interaction event. 
