The galaxy presents a slightly elongated morphology, suggesting it is not perfectly spherical but rather exhibits a degree of oblateness. The light distribution is centrally concentrated, with a bright, relatively compact core, and a somewhat amorphous, less distinct outer region. There is evidence of a faint, diffuse extension or arm-like structure emanating from the central region of the galaxy. Overall, the galaxy appears to be relatively smooth in texture with some presence of internal features. There are signs of minor disturbances in the galaxy’s morphology suggesting it may be a merger with another galaxy. The galaxy has strong light emissions within the green, red, and z bands. The galaxy appears to have a considerable mass and a moderate rate of star formation.
