The galaxy presents an elongated, somewhat cigar-shaped morphology. It displays a smooth, largely featureless light distribution, indicative of an elliptical or lenticular galaxy. The color profile is generally redder, particularly towards the central region, suggesting an older stellar population and reduced star formation activity within the core. There is a slight indication of a disk-like structure, though the disk appears relatively smooth and lacks prominent spiral arms. The galaxy appears relatively isolated, showing no immediate signs of interaction or merging with other galaxies in the immediate vicinity, though a minor disturbance cannot be entirely ruled out. The object is relatively compact in size, but is still a large and massive galaxy in the scheme of the universe. The overall appearance points to a galaxy that has largely ceased forming new stars, and the stellar populations are relatively old.
