The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution without prominent spiral arms or a distinct bar structure. It appears to be dominated by an older stellar population. The color gradient suggests a central bulge region that is yellowish-white, indicating a concentration of evolved stars. There is a slight flattening visible with the longest dimension of the galaxy roughly twice the length of the shortest. There may be a very slight distortion of the light profile which could indicate a recent minor merger. The galaxy exhibits a faint halo that gradually fades into the background. The red color index is relatively low, suggesting a moderate amount of dust attenuation. There is no clear evidence of ongoing star formation in this image.
