The galaxy appears to be an elliptical galaxy, with a smooth, nearly round morphology and no apparent spiral arm structure. The central region exhibits a concentrated and bright yellowish hue, which suggests the presence of an older stellar population. The outer regions of the galaxy fade gradually into the background, indicating a decreasing stellar density with increasing distance from the center. No strong dust lanes or active star-forming regions are visible, consistent with a galaxy that has largely ceased significant star formation. There is a slight hint of a redder color in the outer edges. No signs of ongoing merger activity or major tidal disturbances are observed.
