The galaxy presents as a somewhat elliptical, though nearly round, structure with a smooth light distribution. A bright central bulge is prominent, exhibiting a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy display a fainter, more diffuse blue-ish halo that fades gradually into the background sky. There is a hint of possible minor tidal disturbance or faint arms at the edges of the galaxy. The overall color profile indicates that the central region is dominated by older stars, whereas the outer regions may contain younger, bluer stars, although at a low star formation rate. There is no obvious spiral structure or prominent dust lanes visible.
