The galaxy presents as a moderately bright, elongated spheroid, consistent with an elliptical morphology. The central bulge exhibits a yellowish-white hue, suggesting an older stellar population. Moving outwards, the color transitions to a slightly redder tone in the disk, hinting at a difference in the age or composition of stellar populations within this region. The galaxy demonstrates a relatively smooth texture, lacking any prominent spiral arms or distinct dust lanes. The overall structure suggests a lack of significant ongoing star formation. There is a possible very slight asymmetry within the disk.
