The galaxy presents as an elliptical morphology. The light distribution appears smooth and centrally concentrated, exhibiting a gradual decline in intensity outwards from a bright, reddish core. There are no prominent spiral arms or distinct features suggestive of a disk. The galaxy is elongated, with a relatively high degree of ellipticity. Color gradients are subtle, with the central regions displaying a redder hue that transitions to slightly bluer tones in the outer halo. There are suggestions of minor disturbances in the morphology, but there are no clear signs of any major ongoing merger activity. The galaxy appears relatively isolated and does not appear to be undergoing any major gravitational interactions with neighboring galaxies.
