The galaxy presents an overall smooth appearance, exhibiting a concentrated central bulge. It appears relatively round. The galaxy exhibits a general yellowish hue which is expected for a galaxy at its redshift. The colors could indicate an older stellar population. Faint, diffuse extensions are suspected around the main body of the galaxy, potentially suggesting tidal interactions or merger remnants. The galaxy displays some potential disturbances to its morphology, suggesting either an ongoing or recent merger event. There may be some dust lanes or regions of obscured star formation that contribute to this asymmetry.
