The galaxy appears as a generally smooth and centrally concentrated object. The shape is elongated, with a discernible cigar-like form, rather than perfectly round. There is little to no evidence of spiral arm structure or prominent dust lanes. Color gradients are subtle, exhibiting a yellowish core region which suggests an older stellar population. Fainter blue extensions are visible near the edges, potentially indicative of younger star formation regions. Overall, the galaxy presents a morphology consistent with an elliptical or lenticular galaxy, with a moderate stellar mass. The relative absence of significant ongoing star formation would likely classify this galaxy as part of the red sequence. There appears to be no major ongoing merger events, though minor disturbances cannot be ruled out.
