The galaxy presents a generally smooth and rounded morphology. There is a concentration of light toward the center, suggesting a prominent bulge or core region. The overall color appears yellowish, indicating a population of older stars. While subtle, there may be hints of a faint disk structure surrounding the bulge, but this is difficult to definitively assess. No obvious spiral arm structure or significant dust lanes are apparent. There is no evidence of major merging or tidal disturbances affecting the galaxy's overall shape.
