The galaxy appears as a centrally concentrated object, exhibiting a smooth overall profile. The light distribution suggests an elliptical morphology, leaning towards a circular appearance, though with some deviation from perfect roundness. 

The color profile indicates an older stellar population, with a redder hue dominating the central regions. There might be some minor evidence of disturbance or interaction, observable as a slight asymmetry in the outer regions of the galaxy but it may be an artifact of the observation. Overall, the galaxy shows no signs of major merging events, rather exhibiting a single, cohesive body. 
