The galaxy presents as a relatively smooth, elliptical morphology, with an apparent lack of distinct spiral arm structures. The light distribution appears centrally concentrated, exhibiting a bright, yellowish core that gradually fades into the surrounding halo. The overall shape suggests a moderate ellipticity, deviating slightly from a perfectly circular profile. There is a subtle hint of asymmetry in the outer regions of the galaxy, which could indicate a minor disturbance or interaction. The color profile is dominated by redder wavelengths, suggesting an older stellar population and a relatively low rate of ongoing star formation.
