The galaxy appears as a roughly circular, smooth object with a concentrated central region. It exhibits a somewhat elliptical morphology. The color profile suggests a redder hue overall, particularly in the core, indicative of an older stellar population, though there also seems to be a slight presence of bluer light. The smooth appearance suggests the system is likely an elliptical galaxy, or a spiral galaxy with a dominant bulge and tightly wound arms viewed at a high inclination that obscures detailed arm structure. There is little evidence of active star formation or significant dust lanes.
