The galaxy presents an elliptical morphology, appearing largely smooth and lacking prominent spiral arm structures. Its shape is more akin to a flattened sphere. The central bulge exhibits a concentrated brightness.

There is little indication of significant ongoing star formation, as evidenced by the galaxy's relatively uniform color and absence of bright blue or intensely red regions. The overall color profile suggests a population of older stars, implying that the galaxy is relatively evolved.

While a hint of a disk might be present, the galaxy's dominant feature is its smooth, spheroid-like shape. The potential disk exhibits a subtle asymmetry, leaning towards being cigar-shaped, and lacks distinct features that are a sign of interactions with another object.

The galaxy does not appear to be undergoing a major merger, with the smooth shape and relative lack of disruption suggestive of gravitational stability.
