The galaxy presents as a relatively smooth, elliptical form, exhibiting a high degree of central concentration. The light profile is generally homogenous, with a subtle gradient indicating a bright core. The color appears largely uniform across the galaxy's extent, trending towards the red end of the spectrum. There are no immediately apparent features suggesting strong spiral arms or active star-forming regions. The overall morphology suggests an evolved system dominated by an older stellar population. There is only the slightest indication of any morphological disturbance or tidal interactions, implying relative isolation or past interactions that have since settled. The object’s roundness is quite pronounced; the elongation is almost negligible.
