The galaxy presents an overall elliptical morphology. It exhibits a smooth, diffuse light distribution with a high degree of central concentration. There is no obvious spiral structure or distinct features such as dust lanes or knots of star formation visible. The galaxy's color appears relatively uniform across its extent, with a yellow-orange hue indicative of a relatively old stellar population. There is some asymmetry, which may indicate a minor tidal disturbance and signs of a possible merger. The overall round shape suggests that this is not a disk galaxy observed edge-on, and does not appear to be severely disturbed. The size of the galaxy is moderately large, implying a significant mass.
