The galaxy appears to be a relatively smooth, elliptical system. The core exhibits a yellowish hue, possibly indicating an older stellar population. A subtle color gradient is visible, shifting towards bluer tones in the outer regions, hinting at the presence of younger, hotter stars or ongoing star formation, albeit at a low rate. The galaxy displays an elongated shape, showing that the galaxy is likely somewhat flattened. There is little evidence of significant dust lanes or spiral arm structures. The overall morphology suggests a galaxy undergoing or having completed the transition from a disk-dominated to a spheroid-dominated system. There is a very mild asymmetry in the distribution of light suggesting a possible interaction with another galaxy, but this is not obvious. 
