The galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution with no discernible spiral arms or bar structure. The shape is somewhat elongated, approximating a cigar shape. A color gradient is observed, with a central region appearing more yellowish-white, suggesting an older stellar population, and a slightly bluer hue towards the outer edges, indicating the potential presence of some younger, hotter stars, although they are not prominent. There appears to be a subtle, minor perturbation in the disk, but for the most part it is relatively undisturbed.
