The galaxy presents a primarily smooth, elliptical morphology, with a concentrated central bulge exhibiting a yellowish hue, suggesting a population of older stars. There is some indication of disk-like or featured components, though the overall structure leans heavily toward being smooth. Faint reddish coloration is present, possibly indicating areas of ongoing or recent star formation. The object demonstrates moderate roundness in its shape. Evidence of interactions or mergers is also visible, potentially a relatively minor disturbance. Overall, the galaxy appears as a relatively massive system undergoing complex evolutionary processes.
