The galaxy presents a generally smooth and elliptical appearance. The light is concentrated towards the center, suggesting a prominent bulge. The galaxy appears to be moderately massive with an estimated diameter around 8 kpc. The overall color index suggests the presence of a mix of stellar populations, with a slight prevalence of older, redder stars. There's evidence suggesting a low but non-negligible rate of star formation occurring. The system appears relatively isolated, with no strong signs of ongoing major mergers or significant tidal disturbances. The overall morphology indicates a system that has largely settled into its current form. There may be some minor internal disturbances or interactions occurring but the primary structure remains intact. The galaxy exhibits a notable smoothness in its light distribution, with a high degree of central concentration. The galaxy is not perfectly circular, showing a slight degree of ellipticity.
