The galaxy presents as a flattened, elliptical-like structure. Its core is a bright, concentrated yellowish-orange hue, suggesting an older stellar population dominated by redder giants and supergiants. Progressing outward from the core, the color transitions to a slightly greenish-yellow tinged halo.

The smooth, largely featureless appearance indicates a relative lack of ongoing star formation. There are no prominent spiral arms, dust lanes, or HII regions visible. The galaxy displays a degree of elongation. Minimal signs of major gravitational disturbance, such as tidal tails or irregular shapes are seen, which is consistent with it being mostly undisturbed. The estimated physical size is on the order of tens of thousands of light-years.
