The galaxy presents as a singular object, albeit with some complex morphological features. The primary component exhibits a generally smooth and rounded profile, indicative of an elliptical or lenticular morphology. A secondary, less luminous component is observed adjacent to the primary body, suggesting a possible interaction or merging event. There appears to be significant color variation within the galaxy, with a bright central region. Overall, the observed characteristics point towards a relatively evolved system undergoing some form of dynamic interaction.
