The galaxy presents an elliptical morphology, elongated along its major axis, appearing cigar-shaped with a generally smooth profile. There is a discernible central bulge that is brighter and more concentrated than the outer regions. The color gradient suggests a predominantly older stellar population, indicated by the yellowish hue, especially in the bulge. There is some evidence of a faint, blueish disk component, but it is not sharply defined. No significant signs of ongoing major mergers or tidal disturbances are apparent.
