The galaxy appears to be elliptical, with a smooth, featureless morphology. Its overall shape is elongated, but moderately so, falling into an intermediate roundness category. The galaxy's light distribution is concentrated towards the center, indicating a significant bulge. There is a slight color gradient, with a yellower hue towards the core possibly indicating an older stellar population. No prominent dust lanes or spiral arms are discernible. There is no clear evidence of any ongoing merger activity or major disturbance. The star formation rate appears to be low.
