The galaxy presents an overall elliptical morphology, appearing largely smooth and centrally concentrated. The light distribution is centrally peaked, with a gradual decrease in intensity outwards. The color profile suggests a dominant older stellar population, evidenced by the yellowish-orange hue of the central region. There appears to be a slight asymmetry in the outer regions of the galaxy, with a subtle extension or tidal feature detectable on one side of the main body. This could indicate a past or ongoing minor interaction or merger event. There are areas of blue light present, especially in the disturbed regions, implying star formation, although this appears to be occuring at a low rate. The galaxy does not exhibit a clear spiral arm structure, but could be a disturbed spiral. Overall, the galaxy exhibits characteristics consistent with an early-type galaxy, with a possible ongoing minor merger.
