The galaxy presents as an elliptical morphology, although it is not perfectly spherical, appearing somewhat elongated. It exhibits a smooth light distribution with a dominant central bulge. There are no clearly distinguishable spiral arms or a prominent disk structure. The galaxy appears to be of intermediate size and mass, with a moderate rate of star formation activity. There are no signs of a major ongoing merger, although a minor disturbance or interaction cannot be entirely ruled out given the slightly irregular shape. The color of the galaxy is skewed towards the red end of the spectrum, indicating an older stellar population. The core is very concentrated.