The galaxy presents as a relatively smooth, centrally concentrated object. Its shape is largely elliptical, appearing mostly round. There is little evidence of spiral arm structure or significant dust lanes. The central region displays a brighter, yellowish hue, suggesting a higher concentration of older stellar populations. The outer regions exhibit a bluer color, potentially indicating the presence of some younger stars, albeit less prominent. Overall, the galaxy appears to be a fairly relaxed system without any significant disturbances. A slight asymmetry is observed, but no definitive signs of ongoing or recent merger activity are apparent.
