The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and featureless morphology. Its overall shape is elongated, with an apparent axis ratio suggesting an oblate spheroid. The central region is the brightest part of the galaxy and is a warm white color, indicative of a high concentration of older stars and a potential lack of significant ongoing star formation. The galaxy gradually fades away from the core into the background, with what appears to be a subtle color gradient in the outer regions, shifting toward slightly bluer hues. This could indicate a small amount of younger, bluer stars in these areas, or subtle dust lanes obscuring the redder light from older stars. There is no evidence of spiral arms or a bar structure, and no obvious signs of recent or ongoing major mergers, or tidal disturbances.
