The galaxy presents as a somewhat amorphous structure with a concentrated central bulge exhibiting a yellowish hue. Fainter, diffuse extensions emanate from this core, displaying a bluer color profile, suggestive of ongoing star formation. While a distinct spiral arm structure is not readily apparent, there's a hint of asymmetry, possibly indicating a disturbance or interaction event. The overall light distribution suggests a substantial stellar mass. The galaxy's moderately high redshift indicates it is a significantly distant object, observed in its past state. There may be an actively forming population of stars in the outer regions and/or a weak active galactic nucleus.
