The galaxy presents as a moderately bright, elliptical structure. The core region exhibits a strong concentration of light, appearing nearly white, indicative of an older stellar population. There is a gradual decrease in light intensity moving outward from the central bulge. The galaxy appears to be generally smooth in texture, lacking prominent spiral arms or distinct features. The overall shape is elongated, suggesting a classification between spherical and highly flattened elliptical. There is a subtle color gradient from the central bulge towards the outer regions, with a slight shift towards redder hues. Possible minor disturbances, like a small tidal tail, are present at the bottom of the galaxy. The light emitted suggests a relatively low rate of ongoing star formation.
