The galaxy presents as a somewhat elliptical, smooth object, exhibiting a predominantly yellow-orange hue concentrated in the central region. This suggests a significant population of older stars. While the majority of the galaxy appears featureless, there are hints of a very faint, diffuse disk extending outwards. There may also be an ongoing minor disturbance, but overall, the galaxy doesn't appear to be undergoing any major mergers or interactions based on the current image data. The galaxy presents a generally uniform, non-complex structure from this vantage point.
