The galaxy presents as an elliptical morphology, elongated along a major axis. The central region exhibits a high surface brightness, suggesting a dense concentration of stars. The light profile appears smooth, with no prominent spiral arms or dust lanes visible. The outer regions of the galaxy fade gradually into the background, indicating a decreasing stellar density with increasing radius. There is little evidence of ongoing star formation within the galaxy. The overall color of the galaxy appears to be somewhat redder in comparison to typical spiral galaxies, potentially indicating an older stellar population. The galaxy's shape could suggest a relatively high degree of rotational support or perhaps an ongoing or past minor merger event, though further analysis would be required to confirm such hypotheses.
