The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central region, with a gradual decrease in luminosity towards its outer edges. The shape appears mostly round with a slight ellipticity. There is little evidence of significant dust lanes or spiral arm structures within the galaxy's morphology. Based on the light profile, this object is likely an early-type galaxy. The galaxy appears to be isolated, with no immediate signs of interaction or merging with other galaxies. There may be a hint of a minor disturbance in the outer regions, but this is difficult to confirm due to the resolution of the image. The galaxy exhibits a moderately blue hue, suggesting the presence of some ongoing star formation, albeit at a relatively low rate. The overall structure suggests a galaxy that has largely completed its star formation history, transitioning towards a quiescent state.
