The galaxy appears as a relatively smooth, elliptical object. The light distribution suggests a high degree of central concentration with a gradual decrease in luminosity outwards, consistent with an elliptical morphology. There's no obvious spiral arm structure or dust lane visible in this image. The galaxy has a roughly circular shape, indicating it is likely viewed close to face-on. There may be a very slight asymmetry or a minor disturbance suggesting a past interaction, but it is difficult to determine with certainty from this image alone. The colour profile suggests a dominant population of older stars, implying a relatively low rate of on-going star formation. The galaxy's reddish hue is indicative of this older stellar population.
