The galaxy presents a diffuse, somewhat amorphous morphology. It exhibits a dominant central bulge region, with a significant fraction of its light concentrated there. The overall shape appears to be somewhat elliptical, tending toward round, although not perfectly spherical, with some irregular features. There's an apparent lack of well-defined spiral arm structures. The light distribution appears relatively smooth, suggesting a relatively evolved system. The color indices suggest a population dominated by older stars, though star formation may still occur in relatively low levels. There is a potential for ongoing or past minor merger activity, as there are some suggestions of disturbance in the galaxy's structure. The estimated size implies it is a fairly large galaxy, typical of galaxies that stopped forming stars a long time ago.
