The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology with a bright core. The color profile suggests a population dominated by older stars, with a yellowish-white hue, and possible presence of redder stars in the galactic bulge. There is no apparent spiral structure, and the light is smoothly distributed outwards from the core, indicating a general lack of significant dust lanes or recent star formation. The object displays a relatively high degree of symmetry, lacking any obvious tidal features or indications of recent major merger activity, although a very faint, minor asymmetry cannot be ruled out at this resolution. The galaxy's rounded appearance indicates it is not highly inclined relative to our line of sight.
