The galaxy presents a generally smooth, elliptical morphology. It appears relatively round, with a slight elongation that could suggest a cigar-like shape upon closer inspection. The galaxy's light profile is centrally concentrated, with a gradual decrease in intensity towards its outer regions. The core exhibits a brighter, possibly more active region. While appearing mostly homogenous, a hint of disturbed structure is visible, suggesting a past or ongoing minor interaction with another galaxy, or perhaps internal dynamic processes. Overall, the galaxy appears to be a relatively mature system, potentially with a low star formation rate, as indicated by its smooth, redder appearance. There is a possibility of it being in the process of merging.
