The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that dominates the light profile. The light becomes more diffuse as it moves outward from the center, suggesting a lack of prominent spiral arm structures. There is a very slight asymmetry in the outer halo of the galaxy. The galaxy appears to be generally isolated, without signs of significant tidal interactions or ongoing mergers. The object is a yellow hue, indicating older stellar populations and lower levels of on-going star formation. It has no spiral arms and no dust.
