The galaxy presents as an elongated, likely disk-shaped system, viewed at a high inclination, potentially near edge-on. The central bulge region appears more luminous and has a yellowish hue, suggesting an older stellar population. The outer disk exhibits a bluer color, indicative of ongoing star formation. There are no obvious signs of a recent major merger, although the presence of some minor asymmetries cannot be completely ruled out from this image alone. The galaxy displays a relatively smooth morphology, but there is possible slight disturbance or tidal interaction present. Further spectroscopic analysis would be needed to fully classify the galaxy's type and star formation history.
