The galaxy presents as a lenticular or possibly an elliptical galaxy, exhibiting a generally smooth morphology. The object is elongated, appearing more cigar-shaped than circular, with a relatively high degree of central concentration. There's a distinct color gradient visible, transitioning from a warmer, yellowish hue at the core to cooler, bluish tones in the outer regions. No prominent spiral arms or significant dust lanes are readily discernible. The overall structure suggests an evolved system where star formation may be subdued, consistent with a population of older stars dominating the central region. There are no obvious signs of recent major merger events or tidal disturbances.
