The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated light profile. The core displays a yellowish hue, suggestive of an older stellar population. There is a lack of prominent spiral arms or distinct dust lanes. A slight, subtle elongation is present, but it is predominantly rounded in shape. Overall, the galaxy shows no obvious signs of ongoing major merger activity or tidal disturbances, though some minor irregularities cannot be entirely ruled out.
