The galaxy presents as an elliptical morphology, exhibiting a smooth, relatively featureless profile. Its shape is elongated, approximating a cigar-like appearance rather than a perfectly circular form. The light distribution appears to be centrally concentrated, diminishing towards the outer edges. The color gradient shows a yellow-orange hue, suggesting a stellar population dominated by older, redder stars, with likely suppressed ongoing star formation within the galaxy. There is no discernible spiral structure or significant dust lane present in this image.
