The galaxy appears relatively compact, approximately circular in projection, with an estimated effective radius of about 7.6 arcseconds. Its color indices suggest a likely spiral or irregular morphology, with the presence of some star formation regions. The galaxy's visual appearance is disturbed, showing evidence of gravitational interaction or recent merger activity. A minor tidal tail or distortion extends outwards, indicating possible interactions with a companion galaxy, or the remnants of such. Overall, the system presents as a moderately perturbed galaxy with ongoing or recently concluded interaction.
