The galaxy presents as an edge-on spiral or lenticular type. A central bulge dominates the visual appearance with a smooth, concentrated light profile. A disk is observed, appearing relatively thin and featureless, suggesting a lack of significant ongoing star formation. The bulge exhibits a yellowish-white color, indicative of an older stellar population. The disk appears to be more red than blue, implying a mix of stellar populations, and perhaps modest dust obscuration. There is no obvious evidence of spiral arm structure. There are no signs of strong tidal interactions or major mergers in the image. The galaxy’s overall morphology suggests a relatively evolved system, potentially transitioning to, or already existing as, a more quiescent state.
