The galaxy presents as an elongated, cigar-shaped system. Its overall color profile exhibits a reddish hue, indicative of an older stellar population and potentially significant dust obscuration. There is a smooth light distribution, with the highest intensity toward the galaxy's core. Fainter blue tones are present at the edges of the galaxy, which could indicate younger stellar populations or regions of ongoing star formation at the outer reaches of the galaxy. No prominent spiral arms or bar structures are discernible; rather, the galaxy's morphology suggests an elliptical or lenticular type. There is no noticeable sign of merging or tidal disturbances.
