The galaxy exhibits a generally smooth morphology, with a shape that is neither perfectly round nor significantly elongated, appearing somewhere in between.  There is a slight asymmetry in the luminosity profile, but no strong evidence of major disturbances due to mergers or interactions is readily apparent.  Faint, diffuse outer regions are visible, and the color profile suggests a relatively evolved stellar population. The central region shows a subtle increase in intensity. Evidence suggests it is a galaxy with a moderate stellar mass and a relatively low star formation rate.
