The galaxy appears as a relatively smooth, centralized concentration of light. Its overall shape is somewhat elliptical, though it tends towards a more circular morphology. There is no apparent disk or spiral structure. The color profile suggests an older stellar population, with a yellowish-white hue dominating the light emitted. There is very little evidence of ongoing star formation, as indicated by the lack of blue color, thus indicating a relatively passive galaxy. There are no signs of tidal tails or merging activity, suggesting it is a relatively isolated system not currently undergoing major interactions with other galaxies. Any disturbances seem to be minor, and this galaxy appears to be relatively undisturbed.
