The galaxy presents as a somewhat elliptical, but close to round, morphology. A smooth, centrally concentrated luminosity profile suggests the galaxy is dominated by an older stellar population, with a likely spheroidal structure and little to no visible spiral arm structure or dust lanes. There is a gradual decrease in surface brightness from the core outwards to the edge of the galaxy. The color appears yellowish, indicative of a redshifted spectra with a low to moderate star formation rate. No recent merger events are evident, which could indicate the galaxy is stable and has evolved through secular processes, however, minor disturbances cannot be ruled out.
