The galaxy presents a generally smooth morphology. There are two main concentrations of light, possibly indicating a galactic nucleus or a similar central structure, with an elongated extension of light above it. The light in the system appears somewhat diffuse. The system does not clearly present any spiral arms or disk-like features. The light distribution is relatively symmetrical and is largely contained with in a radius of approximately 3 kiloparsecs. There are no obvious signs of tidal tails or strong gravitational disturbances that indicate a recent major merger. However, there is a galaxy close by, which could be influencing it. The system is relatively dim, with no presence of ongoing strong star formation.
