The galaxy presents as a somewhat elliptical, relatively smooth structure with a yellowish hue concentrated toward the center. Faint, diffuse extensions of bluer material are visible outwards. These extensions might indicate regions of on-going star formation. A minor disturbance or irregularity is seen in the galaxy's shape, possibly indicating a past or ongoing interaction with another galaxy. Based on its color profile, the galaxy is likely composed of an older stellar population with a lower rate of star formation, although some active star formation might be occurring in the outer regions. The mass of this galaxy is likely substantial. 
