This galaxy appears to be an elliptical galaxy. It exhibits a smooth, centrally concentrated luminosity profile with a bright, yellowish core and a fainter, bluish halo. No distinct spiral arms or disk-like structures are discernible. The overall shape is somewhat elongated but close to circular, indicating an intermediate ellipticity. There is no obvious evidence of recent merger activity or tidal disturbances. The color gradient suggests that the stellar population in the core is older and redder compared to the outer regions. There may be evidence of ongoing star formation, though at a low rate, based on the slightly bluer color of the galaxy's halo. Overall, the galaxy seems to be a relatively massive, evolved system.
