The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits an overall elliptical morphology, though not perfectly circular, tending towards an intermediate roundness. There is a lack of prominent spiral arms or distinct disk-like features. The color profile indicates a redder hue in the central regions, suggesting an older stellar population. No significant signs of major mergers or tidal disturbances are immediately apparent, although there may be some minor irregularity in the outer regions, which could indicate a past minor interaction. The object seems to be a massive galaxy with low levels of star formation. 
