The galaxy presents as a centrally concentrated, relatively smooth object with a slightly elliptical shape, suggesting a possible early-type morphology. The galaxy exhibits a noticeable color gradient, appearing bluer towards the center and redder in the outer regions. There is evidence of some disturbance in its morphology. Although the dominant impression is that of a single object, closer inspection reveals some subtle asymmetries in the light distribution that could be indicative of a minor interaction or recent merger event. The overall color suggests a galaxy dominated by older stellar populations, and that the star formation rate is low.
