The galaxy presents a generally smooth morphology with a slightly elongated shape. A central bulge is visible, exhibiting a reddish hue, possibly indicating an older stellar population. Surrounding the bulge is a fainter, more diffuse disk component displaying a bluer color, suggesting the presence of younger, hotter stars and potentially some ongoing star formation. There are hints of disturbances in the galaxy's structure, possibly indicative of a past or ongoing interaction or merger event, resulting in a slight asymmetry. Overall, it appears to be an actively evolving galaxy.
