The galaxy presents a generally smooth morphology, lacking prominent spiral arms or a well-defined disk structure. It appears predominantly elliptical in shape, with a high degree of roundness. The light distribution suggests a relatively homogenous stellar population, lacking significant knots or regions of intense star formation. There is little evidence of tidal features or distortions, suggesting it is not currently undergoing a major merger event. A slight asymmetry and minor disturbance is possible. Color gradients appear subtle across the galaxy, trending towards redder hues.
