The galaxy appears to be an elliptical type, exhibiting a smooth and largely featureless morphology. The light distribution is concentrated towards the center, with a radial decrease in intensity outwards. The galaxy's overall shape is close to circular, with minimal deviation from roundness. There is a slight color gradient, with the central region appearing somewhat yellower and the outer edges becoming slightly bluer, which could suggest the central region may have an older stellar population than the outer parts. A small hint of asymmetry may be present along the edges of the galaxy. There is no evidence of a disk structure or spiral arms. The galaxy shows no prominent signs of ongoing major mergers or significant tidal disturbances.
