The galaxy presents as an elongated structure, likely a spiral viewed edge-on or a highly elliptical galaxy. The central region displays a brighter, concentrated luminosity, suggesting a prominent galactic bulge. The distribution of light across the galaxy is uneven. There is a general color gradient, with the core appearing more yellow/orange and the outer regions showing hints of bluer tones. This may suggest ongoing star formation in the outer regions. There's an asymmetry to the galaxy's structure. One end appears more diffuse than the other, possibly due to tidal interactions or recent accretion events. No strong bar structure is readily apparent.
