The galaxy presents as a generally smooth, elliptical morphology with an apparent lack of significant spiral arm structure. It exhibits a concentrated, bright central bulge that appears yellowish in color, suggesting an older stellar population. The outer regions of the galaxy fade in intensity, displaying a bluer hue. This could indicate the presence of some younger, bluer stars in the disk, but their contribution seems minimal compared to the dominant older population of the bulge. The galaxy's disk is oriented roughly edge-on from our perspective. There are slight irregularities or disturbances in its overall form suggesting a possible recent interaction or merger event, although nothing significant enough to radically disturb its smooth form.
