The galaxy presents as an elliptical, disc-shaped structure with a significantly brighter, concentrated central bulge. The main body exhibits a smooth luminosity profile. The color of the central bulge tends toward a yellow hue, which suggests an older stellar population that likely lacks ongoing significant star formation. The outer disc of the galaxy exhibits a slight blueish tint, implying the presence of younger stars, albeit with a very low star-formation rate. The galaxy displays a slight degree of ellipticity. The shape is neither perfectly round nor elongated into a cigar shape, but something in between. There is evidence of potential disturbances in its structure, but no signs of any major mergers. This suggests that the galaxy is relatively settled but may be experiencing minor interactions or past events.
