The galaxy presents as a fairly concentrated object, exhibiting a morphology tending towards an elliptical or lenticular classification. The light distribution appears smooth with a centrally concentrated brightness profile suggesting an older stellar population. There is a slight elongation in its overall shape, but no distinct spiral arm structures are discernible in this image. The galaxy displays a color gradient, appearing slightly bluer in its outer regions and redder towards the core, which could indicate ongoing star formation in the outer regions, or simply dust in the inner regions obscuring bluer light. There may be some minor disturbances in the galaxy's shape suggesting recent or ongoing interactions with another object. 
