The galaxy presents a primarily smooth morphology. There is a central concentration of light, suggesting the presence of a bulge. The overall shape appears to be elliptical, with a high degree of roundness. There is little to no evidence of spiral arm structure or a well-defined disk. The color profile indicates a relatively red population, which could be indicative of older stars. The image does not reveal any significant signs of ongoing mergers or major disturbances, although minor disturbances cannot be ruled out based on the current data. The galaxy appears relatively isolated, without any close companions. Overall, it is consistent with a galaxy with minimal active star formation.
