The galaxy presents as an elliptical morphology, with a smooth, featureless appearance. Its shape is elongated, appearing cigar-shaped. There's a clear central bulge, brighter and more concentrated than the surrounding areas, with the color distribution showing a yellowish hue. This suggests an older stellar population within the bulge. Moving outwards from the core, the light gradually diffuses, indicating a lower stellar density in the outer regions. No obvious spiral arm structure or dust lanes are visible. The galaxy does not appear to be undergoing any major merging events or experiencing significant disturbances.
