The galaxy presents an elliptical morphology, with a smooth, featureless light distribution, indicating it is likely an early-type galaxy. The object appears elongated, though it is generally rounded. The central region exhibits a yellow hue, possibly indicating an older stellar population. Some blue can be observed, which may indicate the presence of ongoing star formation, but in a low capacity. There is no obvious spiral structure, though faint signs of disturbance may be present, potentially due to a minor interaction or merger in its past. The majority of the galaxy is likely composed of older stars.
