The galaxy presents as an elliptical morphology, appearing smooth and relatively featureless. Its shape is elongated, showing a significant deviation from a perfectly circular profile, trending towards a cigar-like appearance. The color gradient indicates a higher concentration of older stellar populations. There is no prominent dust lane or spiral arm structure detectable in the image. The light distribution within the galaxy appears concentrated towards the center, consistent with the characteristics of an elliptical galaxy. There does not seem to be evidence of any ongoing merger events or major disturbances in the overall structure, although subtle tidal features cannot be completely ruled out due to the image's resolution. The integrated light suggests that the galaxy possesses considerable luminosity.
