The galaxy presents as a somewhat elongated, lens-shaped structure. The central bulge is prominent and exhibits a smooth, diffuse appearance with a concentrated bright core. The color of the bulge appears to be generally yellow to orange, suggesting an older stellar population. Fainter, bluer regions extend from the core, primarily along the edges and extending into the surrounding space. There may be some evidence of disk-like structure or tidal tails. The lack of defined spiral arms suggests that if this galaxy were a spiral, then they are very tightly wound. Based on the overall light distribution and structure, it is likely a massive galaxy. There are no visible signs of a major merger, though the irregular shape suggests minor interaction.