The galaxy presents as a centrally concentrated, relatively smooth object. Its overall shape appears to be somewhat elliptical, though close to circular. The core exhibits a bright, yellowish hue, suggesting an older stellar population is dominant in the galactic center. The light gradually fades towards the outer regions of the galaxy, where a slight red shift is detected. There is little evidence of distinct spiral arm structures or significant dust lanes. No obvious signs of an active galactic nucleus are visible. There are minimal signs of recent or ongoing major merger activity, though a slight asymmetry might indicate a minor gravitational interaction. Overall, the galaxy appears to be a relatively quiescent system, transitioning away from rapid star formation.
