The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. The light distribution appears elliptical, with an axial ratio suggesting a moderate degree of flattening but deviating significantly from a perfect circle. The galaxy core exhibits a notably high surface brightness, fading gradually into the surrounding halo. Colors indicate a redder spectral energy distribution overall, hinting at a stellar population dominated by older, evolved stars and lower levels of ongoing star formation. There is no apparent spiral arm structure or significant dust lane obscuration within the optical wavelengths captured in this image. No major signs of disturbance such as tidal tails or lopsidedness were observed; suggesting a lack of recent major merger activity.
