The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a moderate elliptical morphology. The galaxy's light profile is generally uniform, with a slight elongation suggesting it is not perfectly spherical. I observe very little evidence of spiral arm structure or significant dust lanes. There is no discernible active galactic nucleus. The color appears to be redder overall, indicative of an older stellar population with lower ongoing star formation. There is a possibility that the galaxy is in the process of a minor merger with a smaller companion or experiencing some tidal disturbance, although the image resolution makes a definitive classification challenging. The galaxy's size can be approximated to be medium in size.
