The galaxy presents as a luminous, relatively smooth structure with an elliptical morphology. Its color profile suggests a dominant population of older stars, indicating a possible early-type classification. There is a subtle elongation, deviating slightly from a perfectly spherical shape. A smaller, less luminous companion object is observed in close proximity, potentially interacting with the primary galaxy. There is no strong evidence of active star formation regions or prominent spiral arms. Overall, the galaxy appears to be in a relatively evolved state with a high estimated mass. There is a possibility of a minor disturbance due to the interaction with the nearby companion.
