The galaxy appears as a moderately luminous, relatively smooth object with a concentrated central bulge. It exhibits a slightly elongated morphology, neither perfectly spherical nor highly flattened. The galaxy displays a color gradient, transitioning from a more yellowish-white core region to slightly redder hues in the outer regions. There is no strong evidence of spiral arm structures or significant dust lanes visible in this image. Minor disturbances may be present, but the overall structure does not indicate a major ongoing merger event. Based on its color and morphology, this galaxy is likely an elliptical or lenticular type. Star formation rates appear to be comparatively low. The galaxy's estimated size is approximately 4 kpc in radius.
