The galaxy exhibits a moderate redshift, indicating a significant distance. It appears to be an intermediate-sized galaxy with a mass comparable to that of the Milky Way. The overall morphology appears to be elongated, more cigar shaped than circular. The light distribution is relatively smooth, but there is some evidence of faint disk-like structure and possible disturbance in the galaxy. There is some evidence of on-going star formation with modest star formation rate. It appears to be relatively isolated, without any clear evidence of interaction or merging with other galaxies.
