The galaxy appears as an elliptical structure with a dominant, concentrated central bulge. The light profile suggests a smooth, featureless morphology, with a high degree of central concentration and a gradual decline in surface brightness outwards from the core. The color is predominantly yellowish-orange, indicative of an older stellar population, with the possibility of ongoing star formation. No spiral arm structures or prominent dust lanes are discernible in this image. The galaxy exhibits a moderate ellipticity, appearing more elongated than perfectly circular. There is no apparent evidence of tidal disturbances or interactions with other galaxies. The overall structure suggests a relatively evolved galaxy, likely an elliptical type.
