The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a concentrated, bright yellowish-white luminosity, suggesting a significant population of older stars. The galaxy appears to have a relatively uniform color gradient outwards from the core, with no obvious spiral arm structures visible. There might be a very slight dust lane, but the image resolution makes it difficult to be sure. The galaxy has a slightly flattened, but largely spherical, shape with very little evidence of tidal disturbances or merging activity.
