The galaxy presents as a relatively smooth, centrally concentrated light distribution. The overall morphology appears elliptical, with an approximate effective radius of 5 kpc. The color profile shows a slight bluing toward the outer regions of the galaxy. There is some indication of minor disturbances in the galaxy’s structure, possibly resulting from a past or ongoing interaction or merger. The integrated light indicates moderate levels of recent star formation activity. The estimated stellar mass of this system is significant. Overall, it appears to be a medium-sized galaxy with some signs of recent or ongoing activity.
