The galaxy presents as an elliptical morphology, with a smooth, featureless appearance. The light distribution is concentrated towards the center, exhibiting a bright, well-defined core that diminishes gradually outward. The overall shape appears more in-between rounded and elliptical than perfectly circular, with a slight elongation along one axis. No distinct spiral arms or prominent dust lanes are discernible in this imagery, suggesting a lack of significant recent star formation. There is no indication of tidal tails or other major morphological disturbances indicative of an ongoing merger, though subtle disturbances may not be detectable at this resolution. The galaxy's redder color index suggests an older stellar population and minimal ongoing star formation activity.
