The galaxy presents as a somewhat diffuse object with a bright, concentrated central region. There are features indicative of a disk-like structure, although they are not sharply defined. The overall light distribution suggests a relatively smooth profile, though some irregular patches are observed, which are suggestive of ongoing or recent interactions. The color index indicates the presence of both older stellar populations and regions of more recent star formation, with the redder components likely dominating the overall light. Morphological analysis suggests the possibility of some disturbances, perhaps due to a minor merger event. The estimated size is within the range expected for galaxies of similar luminosity and redshift.
