The galaxy presents a relatively smooth, elliptical morphology with a concentrated central bulge. There is a subtle disk component, though the dominant feature is the spheroid. The galaxy exhibits a yellow-red hue, suggestive of an older stellar population. The overall structure appears largely undisturbed, showing no signs of major mergers or tidal distortions. There's a hint of spiral structure but not significant. Based on this description, the galaxy is likely a massive, evolved system with a relatively low star formation rate.
