The galaxy presents as a primarily elliptical structure with a smooth, concentrated central bulge. Its overall form is relatively well-defined, showing a high degree of symmetry. The light distribution is dominated by older stellar populations, indicated by the yellow to reddish hues in the central region. There's little evidence of spiral arms or distinct disk structures. The galaxy's light profile appears to gradually fade outwards from the core, with no sharp edges or abrupt changes in luminosity. There's a subtle suggestion of a faint halo or envelope extending beyond the main body of the galaxy, but it's only barely discernible. No significant dust lanes or prominent star-forming regions are apparent within the visible structure. The general impression is that of a quiescent, evolved galaxy, likely with a high mass and low star formation rate.
