The galaxy presents a predominantly smooth morphology, appearing as a somewhat symmetrical elliptical structure. There is no apparent spiral arm structure or a well-defined disk. The central region is characterized by a bright, concentrated nucleus exhibiting a yellowish hue. A slightly less luminous, similarly colored region appears offset to the left, suggesting the potential presence of a second nucleus or a region of intense star formation. The overall color profile suggests a moderate redshift and potentially an older stellar population, with a low rate of star formation. There is a slight possibility of a minor interaction or disturbance influencing its morphology.
