The galaxy presents as an elliptical morphology, appearing mostly smooth in structure. Its color profile suggests a dominant population of older stars, emitting light weighted towards the redder end of the spectrum. The galaxy's round shape indicates minimal rotational support, typical of elliptical galaxies. There are no prominent features such as spiral arms or a distinct disk component are visible. There is a faint light profile around the galaxy, with a slight amount of distortion indicating there may have been a minor merger, but that has mostly settled. Overall, the galaxy appears to be a relatively undisturbed system.
