The galaxy presents a moderately elongated morphology, appearing cigar-shaped in its overall form. The light distribution is centrally concentrated, with a brighter core that gradually fades towards the edges. The color profile suggests a redder population of stars, potentially indicating an older stellar population and reduced ongoing star formation. There may be faint evidence of a disk-like structure, but it is not sharply defined. There is no evidence of significant tidal disturbances or major mergers; however, a subtle asymmetry in the outer regions suggests there could be minor interaction with a smaller galaxy. The overall smoothness and color profile points towards it possibly being an elliptical galaxy.
