The galaxy presents as an elliptical type, exhibiting a largely smooth and featureless morphology. Its overall shape is generally round. The galaxy's color profile appears relatively uniform across its structure, displaying a central concentration of light with intensity gradually decreasing towards the edges. There is a hint of a yellowish hue in the central region, suggesting a population of older stars. No prominent spiral arms, bars, or significant dust lanes are visible. There is no strong evidence of ongoing major merger activity or tidal disturbances in this image, although some minor irregularities cannot be entirely ruled out. The galaxy appears to be a relatively isolated system, with no other galaxies of comparable size in close proximity.
