The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards the outer regions. The core displays a yellowish hue, suggesting an older stellar population. The galaxy presents a generally rounded shape, with no significant indication of spiral arms or a prominent disk structure. There is a slight suggestion of faint extended structure around the galaxy. There is no apparent evidence of ongoing major mergers or tidal disturbances. The galaxy shows a minimal amount of blue light, indicative of low ongoing star formation.
