The galaxy presents as a lenticular or early-type spiral, oriented approximately horizontally in the frame. It exhibits a generally smooth, centrally concentrated light distribution, with a notable lack of prominent spiral arms or distinct dust lanes. The overall color is yellowish-orange, suggesting an older stellar population with a relative paucity of ongoing star formation. The galaxy's shape is elongated, more like a cigar than a disc. The presence of a possible smaller blue galaxy nearby suggests that an interaction may be occurring between the two.
