The galaxy presents as a relatively smooth, elliptical morphology. The central bulge exhibits a concentrated, bright yellow/orange hue, indicative of an older stellar population. The color profile suggests minimal ongoing star formation within the bulge. The outer regions display a gradual decrease in luminosity and a slight shift towards redder tones. There are no apparent spiral arms, bar structures, or significant dust lanes visible. The galaxy appears largely undisturbed, with no signs of major tidal interactions or mergers. There is a slight chance of a minor disturbance, but it's likely stable. The overall structure suggests a evolved galaxy, likely an elliptical with a smooth, rounded shape.
