The galaxy presents as a moderately bright, elliptical structure with an apparent angular size of approximately 2 arcseconds. The morphology appears predominantly smooth, with a high degree of central concentration. There is a subtle elongation, suggesting it is not perfectly spherical, leaning towards an in-between state of roundness. The light distribution exhibits a color gradient, appearing yellower toward the core, possibly indicating an older stellar population and/or dust obscuration. There appears to be a minor disturbance in the structure, but the galaxy does not show strong indications of a major merger event.
