The galaxy presents as a somewhat flattened elliptical form. Its core exhibits a high surface brightness, concentrated in the central region. The light profile appears relatively smooth, with a gradual decrease in intensity moving outward from the core. There is a slight elongation along its major axis. Indications of possible minor disturbances within the galaxy’s structure are subtle, not indicating a major merger event, but rather perhaps a slight asymmetry. The overall color is dominated by yellow and red wavelengths, indicating a population of older stars and a low rate of ongoing star formation within the galaxy. The estimated physical size is a few kiloparsecs in radius, characteristic of an intermediate-sized galaxy.
