This galaxy appears to be a relatively smooth, elliptical system with a high degree of central concentration. The core exhibits a bright, yellowish hue, indicative of an older stellar population. There is a gradual decrease in surface brightness moving outwards from the core, with a more diffuse, bluish halo suggesting the presence of some younger stars.

The galaxy is somewhat elongated, showing a slight deviation from a perfectly circular shape. While largely undisturbed, there is subtle asymmetry. This may point to some minor gravitational interaction. There appears to be little or no discernible dust lane present.

The overall appearance is consistent with a galaxy that is undergoing relatively active star formation.
