The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The galaxy's shape is more elongated than circular, approaching a cigar-like appearance, but most of its distribution is concentrated around the core of the galaxy. There are no obvious spiral arm structures or significant disk features discernible. There is no evidence of current or recent major merger events. Faint light in the G band with higher magnitude indicates that this galaxy may be older. The lack of strong blue emission suggests a relatively low star formation rate, consistent with a more evolved stellar population.