The galaxy presents as a relatively smooth, elliptical object. The light distribution suggests a high degree of central concentration, with a bright, yellowish core fading outwards to a more diffuse, reddish halo. There are no prominent spiral arms or distinct features that would indicate active star formation within a disk. The overall shape appears somewhat elongated, but not extremely so. The color gradient from the core to the outer regions could indicate an older stellar population dominating the outer regions and a mix of intermediate-age stars in the galaxy's center. There is no indication of significant tidal distortions or ongoing merger activity. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
