The galaxy presents as a primarily smooth, centrally concentrated object. Its light profile suggests a high degree of symmetry and a lack of distinct spiral arm features. The galaxy exhibits a yellow hue, which suggests an older stellar population and a relatively low rate of ongoing star formation. The morphology is generally round. There is no clear evidence of a recent major merger, although some minor irregularities are visible in the light distribution, suggesting a possible interaction or accretion event in its past. The object has a soft-edged appearance implying a gradual decrease in stellar density as one moves outward from the center of the galaxy. Overall, the galaxy is most likely an elliptical galaxy, with an estimated size of around 7 kiloparsecs.
