The galaxy presents as an elliptical morphology, appearing predominantly smooth with a concentrated central bulge. There is a slight elongation, giving it a cigar-like shape. The light is brightest in the center, diminishing gradually towards the outer edges. The galaxy appears to be a yellow-red hue, suggesting an older stellar population and a possible lack of significant recent star formation. There is no obvious evidence of spiral arms or a prominent disk structure. Additionally, there are no signs of ongoing major merger events.
