The galaxy presents an elliptical morphology, appearing largely smooth and featureless. The core exhibits a concentrated luminosity, suggesting a high stellar density. The overall color profile leans towards the redder end of the spectrum, indicative of an older stellar population and a relatively low rate of star formation. The shape appears neither perfectly spherical nor significantly elongated, presenting a moderate ellipticity. There's no discernible evidence of ongoing major mergers or tidal disturbances, although the presence of minor asymmetry or subtle disturbances cannot be ruled out based on this image alone. Overall, the galaxy appears to be a relatively evolved system.
