The galaxy presents as an elliptical morphology with a generally smooth profile, exhibiting a high degree of central concentration with a bright, yellowish core. The galaxy extends outwards into a less defined halo region, possibly due to lower surface brightness or increasing distance from the nucleus.

The overall color profile suggests a relatively older stellar population, consistent with its classification as an elliptical galaxy. There are potential indications of minor tidal disturbance or interaction with a smaller companion galaxy, evident in the slight asymmetry and faint extension of the halo to the upper-left side. The primary galaxy exhibits an intermediate roundness, appearing neither perfectly spherical nor highly elongated. No distinct spiral arms or prominent dust lanes are visible.
