The galaxy appears as a smooth, elongated object with a concentrated central bulge. Its overall shape is somewhat elliptical, with a high degree of central concentration and a relatively smooth light distribution. The galaxy displays a color gradient, with the central region appearing more yellowish-white, suggesting an older stellar population. The outer regions are fainter and exhibit a bluer hue, possibly indicating the presence of younger stars or ongoing star formation, although this appears subdued. There is a very subtle hint of a disk-like structure, or potential tidal disturbance, or minor merging event, but it is only marginally visible. The galaxy shows no obvious signs of strong spiral arm structure or prominent dust lanes.
