The galaxy presents as an elliptical morphology, with a smooth, concentrated light profile, indicative of an older stellar population. The galaxy appears generally featureless, with no readily discernible spiral arms or prominent dust lanes. The color appears relatively uniform across the galaxy, tending toward redder wavelengths, suggesting a lack of ongoing star formation and a dominance of older, redder stars. The lack of blue light suggests minimal recent star formation. The galaxy exhibits a high degree of central concentration. The general form of the galaxy is a well-defined ellipse, which indicates that the galaxy's dynamics are probably governed by random orbits rather than a disk. The lack of features, and its smooth structure, suggest it is unlikely to be undergoing any major merging events.
