The galaxy presents as a flattened, elongated structure, indicating an elliptical morphology. The central region exhibits a concentrated, bright yellowish hue, suggesting a dense population of older stars. Progressing outwards from the center, the galaxy transitions to a fainter, bluish color, potentially indicating the presence of younger stars or ongoing star formation in the outer regions. The overall appearance is smooth, with no distinct spiral arms or prominent dust lanes visible. The major axis of the galaxy is significantly longer than its minor axis, further supporting its classification as an elliptical galaxy with a high degree of ellipticity. There is no evidence of any tidal features or obvious signs of recent mergers or interactions with other galaxies. The overall light distribution appears relatively uniform and concentrated, with a smooth decline in surface brightness away from the central region.
