The galaxy presents as an elliptical morphology, with a smooth, concentrated luminosity profile that lacks discernible spiral arm structures or a prominent disk. The galaxy's overall shape is observed to be largely spheroidal, with a high degree of roundness. There appears to be a slight color gradient, with the central region exhibiting a yellow hue, potentially indicating an older stellar population. The outer regions appear slightly bluer, suggesting the presence of some younger stars, though this is less pronounced. There is no indication of any major merger events or significant tidal disturbances. The overall light distribution appears relatively even and symmetric. The source is moderately luminous, with no indications of extremely high star formation activity or a prominent active galactic nucleus, but the galaxy still displays some star formation.
