The galaxy presents a generally smooth, elliptical morphology, appearing quite rounded in shape. While not perfectly spherical, there is a noticeable lack of a prominent disk structure. The light distribution is concentrated toward the center, with a gradual decrease in brightness as we move outwards. The galaxy exhibits a fairly smooth and continuous profile without any obvious signs of strong tidal disturbances or ongoing major mergers. However, there is a slight asymmetry and a hint of disturbance in the outer regions, possibly indicating a minor interaction or past accretion event. Based on its color, the galaxy appears to have an older stellar population, and a comparatively low rate of ongoing star formation. It is a massive object, likely on the order of 10^10 solar masses, and located at a redshift of approximately 0.15.
