The galaxy appears as an elliptical-like structure with a diffuse, smooth texture. Its color is predominantly a yellowish-orange hue, suggesting a population of older stars and a relative lack of ongoing star formation. There's an uneven distribution of light across the galaxy, showing two to three brightened, more condensed regions. These condensations are likely either the galaxy's core with multiple centers, or a possible disturbance indicative of a merger event. There is no clear evidence of spiral arms or a prominent disk structure. The overall morphology suggests a system that is either in the process of merging with another galaxy, or a fairly round system with non-uniform brightness.
