The galaxy presents as a largely featureless, elliptical-like structure. Its core exhibits a concentrated, bright luminosity that diffuses outward, transitioning into a fainter halo. There is no evidence of spiral arms or a distinct disk component visible in the image. The overall shape is almost perfectly round. A very slight asymmetry can be detected along what appears to be its horizontal plane, possibly hinting at minor gravitational disturbances but there are no obvious signs of a merger event. The galaxy's color appears to be shifted towards the redder part of the spectrum with a redshift of 0.118685 which could indicate an older stellar population and/or a significant amount of dust absorption within the galaxy.
