The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a central bulge that dominates the overall light profile, with a gradual decrease in luminosity outwards. The color appears relatively uniform throughout, with a slightly redder hue, suggesting a population of older stars and a lower rate of current star formation. No distinct spiral arm structures or dust lanes are readily apparent. The galaxy shows an elongated shape, indicating that it may be viewed at an angle, not face-on. There does not seem to be any signs of major disturbances or interactions with other galaxies.
