The galaxy appears to be a relatively smooth, centrally concentrated object. There is a slight elongation, suggesting it is not perfectly spherical but rather somewhat elliptical in shape. A faint disk-like structure may be present, although it is not prominently defined. The color profile is relatively uniform across the galaxy, with a tendency toward redder hues overall, and a slightly brighter central bulge. There does not seem to be any ongoing major merging event, tidal tails, or other indications of significant gravitational disturbance, but there is slight suggestion of a faint outer halo. The galaxy's light output indicates that there are some ongoing processes of star formation, at a relatively low rate.
