The galaxy presents as a moderately bright, elliptical-like structure, exhibiting a smooth and relatively featureless morphology. The light profile displays a concentrated central bulge, with a gradual decrease in luminosity towards the outer regions. The color distribution shows a central region dominated by yellowish hues, suggesting an older stellar population and reduced star formation activity. Progressing outward, the color shifts towards slightly bluer tones, implying the potential presence of younger stars or residual star forming regions, though these are not distinctly visible. There is very little evidence of spiral arms or dust lanes, thus supporting its classification as a spheroid galaxy. The overall appearance suggests a system that has largely completed its major star formation phase, with characteristics leaning toward a more evolved galaxy type. There is no obvious presence of strong tidal features, suggesting it has not recently undergone a major merger event, or that any such event occurred long enough ago that the galaxy has settled into its current configuration.
