The galaxy appears to be a relatively smooth, centrally concentrated object. Its morphology is suggestive of an elliptical galaxy, although some disk-like or irregular features cannot be ruled out given the resolution. The object exhibits a color gradient, with a yellowish-white core transitioning to redder hues in the outer regions. This color profile could indicate an older stellar population concentrated in the nucleus, with younger, bluer stars being less prominent or obscured. The galaxy's shape is somewhat elongated, possibly indicating it is an oblate spheroid viewed at an angle. There is no obvious evidence of tidal tails, strong gravitational lensing, or significant ongoing merger activity based on visual inspection, although minor disturbances cannot be completely discounted. Overall, the galaxy presents as a moderately massive system, plausibly at an intermediate stage of its evolutionary history.
