The galaxy presents as a somewhat elongated, cigar-shaped structure. The light distribution is generally smooth, with a subtle concentration toward the central region, though without a distinct, bright nucleus. There's a hint of disk-like structure, with an absence of major distortions or tidal features indicating ongoing or recent major merger activity. It exhibits a yellowish-orange hue, suggesting an older stellar population. The overall morphology suggests a later-type galaxy that is quiescent or undergoing moderate star formation.
