The galaxy presents as a relatively compact and luminous object, exhibiting a largely smooth and rounded morphology. There is no indication of a prominent disk structure or spiral arms within the resolution of the image. The light distribution suggests an elliptical or lenticular classification. 

The object displays a color gradient, appearing bluer towards the central region, transitioning to redder hues in the outer parts. This could be indicative of ongoing or recent star formation occurring primarily in the core, with an older stellar population dominating the periphery. 

There are hints of minor disturbances in the galaxy's shape, although it does not present a clear merging signature or evidence of major disruption. The central condensation is quite pronounced suggesting a centrally concentrated mass distribution.
