The galaxy presents as a relatively smooth, round object. Its color is primarily red, indicating a population of older stars, and has a significant mass. There is a suggestion of very minor disturbances within the galaxy's structure; these could represent the remnants of a past minor merger or tidal interactions, or internal processes driving slight asymmetries. Star formation appears to be suppressed. The galaxy is likely an elliptical galaxy, although higher resolution imaging would be required to confirm the absence of any significant disk structure definitively.
