The galaxy presents a primarily smooth morphology, with a notable central bulge that dominates its structure. The light from the bulge exhibits a yellowish hue, indicating an older stellar population and potentially lower star formation activity in that region. Surrounding the bulge is a fainter, more diffuse disc. This disc exhibits a slightly bluer color than the central bulge, suggesting the presence of younger, hotter stars, and possibly ongoing star formation within the disc. The galaxy's overall shape appears somewhat elliptical, with an apparent oblateness that suggests it may be viewed at an angle. There are hints of minor irregularities or disturbances in the outer regions of the disc, but these features are not clearly defined, indicating no major ongoing merger events. Overall, the galaxy appears to be a relatively massive system.
