The galaxy presents a smooth, elongated morphology, consistent with a highly inclined disk or a lenticular type. The central bulge appears prominent and exhibits a yellowish-orange hue, suggesting an older stellar population. The outer regions of the disk are less defined, with a faint bluish tinge, potentially indicating some ongoing star formation. There is no obvious evidence of spiral arm structure or strong dust lanes within the resolution afforded by the image. No major signs of tidal disruption or interaction with nearby galaxies are readily apparent, although the galaxy appears slightly asymmetrical. Overall, it is a relatively massive galaxy, possibly transitioning from a more actively star-forming phase to a more quiescent state.
