The galaxy presents as an elliptical morphology, appearing largely smooth in texture. The color profile suggests a higher concentration of older stellar populations, evidenced by the central yellowish hue. The galaxy displays an elongated shape, appearing closer to an elliptical cigar shape than a perfect sphere. Some faint blue is present in the outer region of the galaxy, indicating that it has a very low number of young, hot stars. No strong evidence of spiral arm structure or a prominent disk component is readily apparent. There are no major indications of interaction or merger events with other galaxies, although there may be some indications of a minor disturbance in the morphology.
