The galaxy presents as an elongated, spindle-shaped structure. The central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population, possibly an older bulge. Moving outwards from the core, the light gradually fades, displaying a smoother appearance without distinct spiral arm features. The overall color gradient shifts from a more yellowish central hue to slightly bluer tints in the outer regions. There may be minor disturbances present, but the galaxy appears to be relatively isolated and unperturbed in its morphology. The galaxy’s major axis appears to extend roughly twice its minor axis, suggesting a highly flattened ellipsoidal shape.
