The galaxy exhibits a predominantly smooth morphology, with a slight degree of irregularity suggesting the possibility of a minor interaction or disturbance. The galaxy's central region presents a bright, concentrated core, surrounded by a more diffuse halo. The overall shape is somewhat elliptical, approaching a rounded appearance. The color gradient indicates a generally older stellar population, with a redder hue dominating. However, there are hints of bluer regions embedded within the galaxy, likely indicative of pockets of more recent star formation. There is a notable absence of well-defined spiral arms or a distinct disk structure. Overall, the galaxy appears to be a relatively massive system, exhibiting low-level star formation activity, and showing signs of a past merger event.
