This galaxy presents as an elongated, elliptical morphology. Its central bulge exhibits a bright, concentrated luminosity, suggesting a high density of older stellar populations. The galaxy appears relatively smooth, lacking prominent spiral arms or distinct dust lanes. The color profile indicates a redder hue, potentially indicative of an older stellar population and lower ongoing star formation activity. The overall structure suggests a classification towards an elliptical galaxy, with a possible slight distortion from a perfect elliptical shape, hinting at a possible past interaction or minor disturbance.
