This galaxy presents as an elongated, spindle-shaped system, possibly an edge-on disk galaxy or an elliptical galaxy with a prolate shape. The central bulge is a prominent, concentrated region of light, exhibiting a yellowish-white hue, which may indicate an older stellar population. Moving outward from the center, the luminosity gradually decreases. The color shifts towards a bluer tint, most notably at the apparent edges of the galactic structure, potentially indicating more recent star formation or a younger population of stars in the outer regions. There is no obvious spiral arm structure visible. The smooth, tapering morphology suggests a relatively undisturbed system, although subtle irregularities in the outer regions cannot be entirely ruled out given the image resolution.
