The galaxy presents as a somewhat diffuse object with an apparent elongated morphology. Its color is predominantly yellowish, suggesting an older stellar population. There may be evidence of interaction or a potential merger event in progress. The object seems to have a primary nucleus with a fainter secondary component situated nearby, possibly a smaller galaxy being accreted. The overall structure is moderately smooth, with a high degree of central concentration. There are minimal indications of spiral arm structures or active star forming regions.
