The galaxy presents as a moderately bright, relatively compact object. Its overall shape appears largely elliptical, with a high degree of central concentration. There's a noticeable color gradient, transitioning from a brighter, somewhat bluer core region to a slightly fainter, redder outer halo. No distinct spiral arm structures or prominent dust lanes are discernible. The overall smoothness of the light distribution suggests it's likely an early-type galaxy with a relatively old stellar population and suppressed star formation. There are no obvious signs of tidal interactions or ongoing merging events.
