The galaxy presents a somewhat elliptical morphology, appearing as a flattened spheroid when viewed from our vantage point. The light distribution suggests a relatively smooth profile with a concentrated central bulge that transitions into a fainter, extended disk. The color gradient shows a central region that is yellowish-white, indicating an older stellar population, transitioning to bluish hues in the outer regions of the disk, which indicates possible ongoing star formation. Subtle dust lanes may be present within the disk, though the image resolution makes it difficult to confirm. There are hints of asymmetry in the outer edges, which could suggest gravitational interactions with another galaxy. The galaxy shows no signs of any major merger.
