The galaxy presents as a single, relatively smooth object with a concentrated central region. Its overall shape appears elliptical or spheroidal, exhibiting high degree of roundness. The galaxy displays a distinct reddish-yellow hue, suggesting an older stellar population and a lower rate of ongoing star formation. There is no strong evidence of spiral arms or a distinct disk structure. There are no apparent signs of tidal disturbances or ongoing mergers with other galaxies. The light profile appears relatively even, decreasing smoothly from the core outwards, with no significant irregularities or bright knots visible. Overall, the galaxy appears to be a massive, quiescent system, possibly a lenticular or elliptical galaxy observed at a considerable distance.
