The galaxy appears as a centrally concentrated object with a generally smooth morphology. The light distribution indicates a spheroidal shape, with no apparent spiral arm structures or prominent disk features. The core region exhibits a bright, relatively uniform yellow-white color, suggesting an older stellar population. There is a slight color gradient from the core outwards, with a subtle reddening in the outer regions. This may indicate a difference in stellar populations, dust content, or metallicity as a function of distance from the galactic center. Faint, diffuse light extends outwards from the central region, fading gradually into the background. There are no signs of active galactic nuclei (AGN) activity, such as jets or strong emission lines. The overall appearance suggests an evolved galaxy with a relatively low star formation rate. Possible signs of minor tidal disturbances are present, but there does not appear to be any evidence of recent major merger events or strong interactions with other galaxies.
