The galaxy presents as a slightly tilted disk-shaped structure. Its core region exhibits a concentrated, bright yellowish-white hue, suggesting an older stellar population or potentially an active galactic nucleus. Surrounding the central bulge, a fainter, bluish disk is visible, indicating the presence of younger, hotter stars and possible ongoing star formation. The overall morphology leans towards a smooth appearance, but subtle irregularities within the disk structure may imply minor disturbances or interactions. The galaxy lacks a clear, dominant spiral arm structure, which suggests it may be an intermediate spiral or possibly a lenticular galaxy. The color gradient from the core to the outer regions signifies varying stellar populations and star formation activity across the galaxy.
