The galaxy presents as a relatively smooth, elliptical morphology. The light distribution is centrally concentrated, exhibiting a high degree of roundness. There are no obvious signs of significant disk-like structures, tidal tails, or strong morphological disturbances indicative of major mergers. The color index, estimated from the red, green, and blue channels, suggests an older stellar population, likely dominated by evolved red and yellow stars. Star formation activity appears low, indicated by the lack of bright blue regions. The size is compact. There's possibly a minor gravitational interaction occuring, but more data is needed. The estimated mass is substantial, which supports the observed morphology.
