The galaxy appears as a relatively compact, centrally concentrated object. The morphology seems largely smooth, with the light profile gradually decreasing from the center outwards. There is little evidence of spiral arms or a distinct disk structure. The galaxy exhibits an elliptical shape, appearing somewhat elongated rather than perfectly spherical. There is a slight color gradient, with a more reddish hue towards the central region, possibly indicating an older stellar population concentrated in the core. The outer regions exhibit a bluer color. No significant tidal features or signs of major recent mergers are apparent, although there might be some minor irregularities in the outer isophotes suggesting possible past interactions. Star formation is likely present, but at a relatively moderate level.
