The galaxy presents as a somewhat diffuse, yet centrally concentrated, luminous object. Its overall morphology appears to be relatively smooth, though not perfectly spherical. There may be a faint, somewhat flattened disk structure oriented horizontally relative to the frame. The central region displays a yellowish-orange hue, potentially indicating a population of older stars, dust obscuration, or a combination of both. The outer regions show hints of blue-green coloration, suggesting some ongoing or recent star formation, though it is not pronounced. There are potential signs of minor disturbances in the galaxy's morphology which may be due to minor interactions with another object. The object does not show any signs of a strong merger.
