The galaxy presents as a single, largely homogenous structure. It appears elliptical in shape, with no discernible spiral arms or bar. The light is concentrated towards the center, with a smooth falloff towards the edges, indicating a bulge-dominated morphology. The galaxy exhibits a yellow-red hue across its surface, suggesting an older stellar population. Its fairly round shape does not show any major signs of tidal disruption or interaction, although there appears to be a very minor disturbance along the outer edge on its left side. The galaxy appears to be a relatively large, passive elliptical galaxy with ongoing, but low, star formation.
