The galaxy presents as a centrally concentrated object, exhibiting a smooth, largely featureless morphology. The light profile appears approximately circular, with no apparent elongation or significant deviations from roundness. The core region displays a bright, yellowish hue, possibly indicating an older stellar population. A surrounding, fainter halo or extended envelope is visible, showing a subtle gradient in color, transitioning toward greenish tones at its periphery. The overall smooth appearance suggests a lack of ongoing major merging activity or significant disturbances in its structure. Faint light is visible throughout the central regions of the galaxy, suggesting an average star formation rate. The color suggests that this is a massive galaxy.
