The galaxy presents as a flattened, elongated spheroid with a major axis significantly larger than its minor axis, classifying it morphologically as likely an elliptical galaxy or a lenticular galaxy viewed edge-on. The central region displays a concentrated, bright, yellowish hue suggesting an older stellar population likely dominated by evolved stars. Progressing outwards from the core, the luminosity diminishes gradually into a less distinct outer region exhibiting a reddish tint. There are no apparent spiral arm structures or dust lanes visible, supporting the classification as elliptical or lenticular. The galaxy does not show any signs of significant tidal disturbances or ongoing major mergers based on visual inspection of the surrounding structure. The color gradient implies a declining rate of star formation from the core outwards. 
