The galaxy presents a somewhat elliptical morphology, with a centrally concentrated bulge exhibiting a yellow-orange hue, suggestive of an older stellar population. The primary body of the galaxy appears relatively smooth, lacking prominent spiral arm structures or strong dust lane features. A faint, diffuse, blue-tinged extension emanates from the main body, possibly indicative of a tidal tail or a region of recent or ongoing star formation activity. Overall, the galaxy appears to be a system with intermediate to high mass, and a relatively quiescent star formation rate. There is a hint of a possible interaction or merger event in the relatively recent past, given the asymmetric feature.
