The galaxy presents a generally smooth morphology, with a high degree of central concentration. It exhibits an elliptical shape, with an axis ratio indicating it is close to round. The color appears predominantly redder, suggesting an older stellar population. There is no distinct disk structure or spiral arm pattern visible. No significant tidal features or distortions are apparent that would indicate an ongoing or recent merger event. The light distribution appears relatively uniform, without pronounced star-forming regions. The estimated size appears to be substantial. The lack of blue color further suggests low ongoing star formation.
