The galaxy presents as a relatively smooth, disk-like structure, with a notable central bulge that appears quite bright. The disk component exhibits a subtle blueish hue, suggesting the presence of younger, hotter stars and ongoing star formation. There may be slight disturbances in the overall structure of the galaxy. Based on the light profile, it is not a perfectly smooth elliptical. Evidence of a central concentration is also visible. The galaxy's shape is closer to edge-on rather than face-on as it appears elongated.
