The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing nearly spherical and featureless. Moving outwards from the center, the light gradually diminishes in intensity. Subtle deviations from perfect elliptical symmetry are observed, with some suggestion of a faint, disturbed disk component. There are hints of asymmetry in the outer regions, possibly indicating minor gravitational interaction or tidal disturbances. The color profile suggests a population dominated by older stars, evidenced by the redder hues, with indications of very low star formation activity within the galaxy, but this does not appear to be ongoing. Overall the galaxy appears to be of significant size and mass.
