The galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated light distribution. Its color profile suggests a slightly older stellar population, with a yellowish-orange hue. The galaxy displays a moderate degree of roundness, but with a significant fraction exhibiting an intermediate form between perfectly round and elongated. There is no clear evidence of significant tidal disturbances or ongoing major mergers, though minor disturbances cannot be ruled out. Overall, the galaxy presents as a relatively undisturbed, evolved system.
