The galaxy appears to be an elliptical galaxy, exhibiting a relatively smooth and featureless morphology. Its shape is neither perfectly round nor highly elongated, tending more toward an intermediate form. There is no discernible spiral structure or bar visible. Light distribution appears centrally concentrated, gradually decreasing with radial distance from the core. The galaxy's color is predominantly yellowish-white, suggesting an older stellar population with relatively low ongoing star formation, and a moderate mass estimate. There are indications of possible minor disturbance, but no major merger is apparent based on this image. The galaxy appears relatively isolated, without strong evidence of tidal interactions or ongoing mergers with other significant objects in the immediate vicinity.
