The object presents as a moderately luminous galaxy, with a morphology that is generally smooth and somewhat elliptical. It appears to be a relatively evolved system. The galaxy exhibits a mostly uniform color profile with a slight central concentration of luminosity. There is a suggestion of minor distortions present, possibly indicating a weak tidal interaction or internal instability. Based on its color indices, star formation rates are likely low to moderate. There is no strong evidence of prominent spiral arms, bars, or dust lanes. Overall, the galaxy is a fairly typical example of a relatively massive system.
