The galaxy presents as an elliptical morphology with a smooth overall appearance. It exhibits a concentrated central bulge, which is luminous and appears yellowish, indicative of an older stellar population. The galaxy lacks prominent spiral arms or a well-defined disk structure. There is a subtle color gradient from the center outwards, with the outer regions appearing slightly bluer, suggesting the presence of a small population of younger, hotter stars, albeit subdued. The galaxy appears relatively isolated with no obvious signs of ongoing major merger activity or tidal disturbances. It is moderately redshifted, placing it at a considerable cosmological distance. The effective radius appears to be a few kiloparsecs across. The estimated mass is substantial, roughly 10^10 solar masses. The star formation rate appears to be fairly low.
