The galaxy presents a relatively smooth, concentrated central region with a yellow-orange hue, indicating an older stellar population. There's evidence of a secondary, bluer component offset from the main body, suggesting either a smaller, star-forming region within the galaxy or a possible minor merger event. The galaxy appears to be approximately circular in projection, though subtle distortions are present. It exhibits moderate luminosity, with indications of ongoing, though relatively low, star formation activity. The overall morphology suggests a system that is either in the process of merging or has experienced a recent interaction. There appears to be some minor disturbance in the structure. The object is of intermediate mass, not among the most massive galaxies but also not a dwarf galaxy.
