The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular type, but with a hint of a disk-like structure. The object appears elongated in shape, leaning towards a cigar-like form. The primary light emission is centrally concentrated, with a falloff in surface brightness toward the edges. There appears to be a faint blue hue, particularly in the central region. Evidences suggest minor disturbances, however, it exhibits no signs of major mergers or significant tidal interactions. The star formation rate appears to be relatively low. The galaxy presents as a single, coherent body, with no obvious companion galaxies or extended tidal features.
