This galaxy exhibits a slightly extended morphology. It presents with a centrally concentrated luminosity profile. The object appears to be mostly smooth in structure, but a very faint, diffuse, extended disk is potentially present. There are no clear spiral arm features evident. While the dominant characteristic is a smooth appearance, some subtle disturbances may be occurring; however, the evidence for major merging activity appears to be minimal. It's redshift value suggests a high luminosity profile, and blue color in the DESI imaging further suggests active star formation within the galaxy. The galaxy may be interacting with a neighbor.
