The galaxy appears as a moderately compact object with a roughly elliptical morphology. Its light distribution seems relatively smooth, suggesting a lack of prominent spiral arms or significant clumpy structures. The color is somewhat uniform across the galaxy's body, with a slight tendency toward redder hues, indicative of an older stellar population and/or a degree of dust obscuration. There might be a very slight distortion or irregularity in the galaxy's shape, potentially hinting at a minor past interaction or internal disturbance. Overall, the galaxy's visual characteristics point toward a relatively evolved system with a suppressed star formation rate.
