The object presents as a galaxy with an elliptical morphology. The galaxy appears to be relatively smooth in texture, with a high degree of central concentration. The core exhibits a bright, yellowish hue, suggestive of an older stellar population. Moving outwards from the core, the galaxy's color gradually shifts towards a redder tone, potentially indicating a lower average stellar age or increased dust extinction in these regions. There is a subtle asymmetry in the outer regions, but no major disturbances. The galaxy is moderately sized and has no signs of ongoing mergers or tidal interactions.
