The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high degree of concentration, appearing nearly circular and very bright. Moving outward from the center, the luminosity decreases gradually, with a faint halo or extended envelope of light surrounding the central region. The overall color of the galaxy appears slightly yellowish, suggesting a population dominated by older stars with a low rate of current star formation. There is no prominent evidence of spiral arms or significant dust lanes. A very slight asymmetry may be present in the outer regions, but this could be due to noise or a minor tidal interaction.
