This galaxy presents as a relatively faint, diffuse object. Its overall morphology is somewhat amorphous, lacking any prominent spiral arms or a well-defined central bulge. The light distribution appears fairly smooth, with only subtle variations in surface brightness across the galactic disk, suggesting an absence of significant ongoing star formation. The galaxy exhibits a blueish hue, implying the presence of some younger stellar populations although not a substantial amount. There's some evidence for minor disturbances in the galaxy's structure, potentially hinting at past or ongoing interactions with smaller galactic companions, though a major merger is not apparent.
