The galaxy presents as a centrally concentrated, smooth elliptical or lenticular type. There's a distinct, bright, yellowish core that suggests an older stellar population dominating the central region. The galaxy appears relatively isolated, showing no signs of major disturbances or ongoing mergers, although minor irregularities cannot be entirely ruled out at this resolution. The overall shape is generally round, tending more towards elliptical with a slight elongation. A diffuse halo or envelope is observed, extending outwards from the core, indicative of a well-established and dynamically relaxed system. The color gradient suggests a decline in star formation activity towards the outer regions.
