The galaxy presents as a concentrated, largely homogenous structure. Its morphology appears elliptical, displaying a high degree of sphericity with minimal apparent elongation or distortion. The light distribution is centrally concentrated and diffuse, lacking defined spiral arms or a prominent galactic disk. The color profile is primarily uniform, with a slight bluer hue near the center, possibly indicating the presence of a younger stellar population, and redder hues near the edge, possibly indicating the presence of an older stellar population. The overall appearance suggests a relaxed system, potentially indicative of an early-type galaxy or a bulge-dominated spiral galaxy at moderate redshift. There is no evidence of significant ongoing mergers or major tidal disturbances in the surrounding region.
