The galaxy presents as a moderately luminous object, with a generally smooth and rounded appearance. There is subtle evidence of a disk-like structure, but it does not dominate the morphology. The central region appears somewhat more concentrated in light, suggesting a possible bulge. Indications of recent or ongoing merging activity is suggested by subtle asymmetrical features, suggesting it may be undergoing minor disturbances. There appears to be a generally quiescent star formation rate. The object's overall color suggests a population of moderately aged stars. The estimated physical size suggests this is not a dwarf galaxy, and the mass values place it well within the range of typical large galaxies.
